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Morgado BE, Sicardy B, Braga-Ribas F, Ortiz JL, Salo H, Vachier F, Desmars J, Pereira CL, Santos-Sanz P, Sfair R, de Santana T, Assafin M, Vieira-Martins R, Gomes-Júnior AR, Margoti G, Dhillon VS, Fernández-Valenzuela E, Broughton J, Bradshaw J, Langersek R, Benedetti-Rossi G, Souami D, Holler BJ, Kretlow M, Boufleur RC, Camargo JIB, Duffard R, Beisker W, Morales N, Lecacheux J, Rommel FL, Herald D, Benz W, Jehin E, Jankowsky F, Marsh TR, Littlefair SP, Bruno G, Pagano I, Brandeker A, Collier-Cameron A, Florén HG, Hara N, Olofsson G, Wilson TG, Benkhaldoun Z, Busuttil R, Burdanov A, Ferrais M, Gault D, Gillon M, Hanna W, Kerr S, Kolb U, Nosworthy P, Sebastian D, Snodgrass C, Teng JP, de Wit J. Author Correction: A dense ring of the trans-Neptunian object Quaoar outside its Roche limit. Nature 2024; 626:E2. [PMID: 38228877 DOI: 10.1038/s41586-024-07031-w] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/18/2024]
Affiliation(s)
- B E Morgado
- Federal University of Rio de Janeiro - Observatory of Valongo, Rio de Janeiro, Brazil.
- National Observatory/MCTI, Rio de Janeiro, Brazil.
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil.
| | - B Sicardy
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
| | - F Braga-Ribas
- Federal University of Technology, Paraná (UTFPR/DAFIS), Curitiba, Brazil
| | - J L Ortiz
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - H Salo
- Space Physics and Astronomy Research unit, University of Oulu, Oulu, Finland
| | - F Vachier
- The Institute of Celestial Mechanics and Ephemeris Calculation (IMCCE), Observatory of Paris, PSL Research University, CNRS, Sorbonne University, UPMC University of Paris, University of Lille, Lille, France
| | - J Desmars
- The Institute of Celestial Mechanics and Ephemeris Calculation (IMCCE), Observatory of Paris, PSL Research University, CNRS, Sorbonne University, UPMC University of Paris, University of Lille, Lille, France
- Polytechnic Institute of Advanced Sciences (IPSA), Ivry-sur-Seine, France
| | - C L Pereira
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - P Santos-Sanz
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - R Sfair
- Institute for Astronomy and Astrophysics, Eberhard Karls University of Tübingen, Tübingen, Germany
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - T de Santana
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - M Assafin
- Federal University of Rio de Janeiro - Observatory of Valongo, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - R Vieira-Martins
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - A R Gomes-Júnior
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
- Institute of Physics, Federal University of Uberlândia, Uberlândia, Brazil
| | - G Margoti
- Federal University of Technology, Paraná (UTFPR/DAFIS), Curitiba, Brazil
| | - V S Dhillon
- Department of Physics and Astronomy, University of Sheffield, Sheffield, UK
- Institute of Astrophysics of The Canary Islands, La Laguna, Spain
| | | | - J Broughton
- Reedy Creek Observatory, Gold Coast, Queensland, Australia
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - J Bradshaw
- Samford Valley Observatory (Q79), Brisbane, Queensland, Australia
| | - R Langersek
- Algester Astronomical Observatory, Brisbane, Queensland, Australia
| | - G Benedetti-Rossi
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - D Souami
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
- Observatory of the Côte d'Azur, Lagrange Laboratory UMR7293 CNRS, Nice, France
- naXys, University of Namur, Namur, Belgium
| | - B J Holler
- Space Telescope Science Institute, Baltimore, MD, USA
| | - M Kretlow
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
- International Occultation Timing Association / European Section, Hannover, Germany
- International Amateur Observatory e.V. (IAS), Mittenwalde, Germany
| | - R C Boufleur
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - J I B Camargo
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - R Duffard
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - W Beisker
- International Occultation Timing Association / European Section, Hannover, Germany
- International Amateur Observatory e.V. (IAS), Mittenwalde, Germany
| | - N Morales
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - J Lecacheux
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
| | - F L Rommel
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - D Herald
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - W Benz
- Institute of Physics, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - E Jehin
- STAR Institute, University of Liège, Liège, Belgium
| | - F Jankowsky
- Heidelberg-Königstuhl State Observatory, Heidelberg, Germany
| | - T R Marsh
- Department of Physics, University of Warwick, Coventry, UK
| | - S P Littlefair
- Department of Physics and Astronomy, University of Sheffield, Sheffield, UK
| | - G Bruno
- INAF, Catania Astrophysical Observatory, Catania, Italy
| | - I Pagano
- INAF, Catania Astrophysical Observatory, Catania, Italy
| | - A Brandeker
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - A Collier-Cameron
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, UK
| | - H G Florén
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - N Hara
- Astronomical Observatory at the University of Geneva, Versoix, Switzerland
| | - G Olofsson
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - T G Wilson
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, UK
| | - Z Benkhaldoun
- Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Marrakech, Morocco
| | - R Busuttil
- School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, UK
| | - A Burdanov
- Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA, USA
| | - M Ferrais
- Laboratory of Astrophysics of Marseille, University of Aix Marseille, CNRS, CNES, Marseille, France
| | - D Gault
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - M Gillon
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | - W Hanna
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - S Kerr
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
- Astronomical Association of Queensland, Pimpama, Queensland, Australia
| | - U Kolb
- School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, UK
| | - P Nosworthy
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - D Sebastian
- School of Physics and Astronomy, University of Birmingham, Birmingham, UK
| | - C Snodgrass
- Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK
| | - J P Teng
- AGORA Observatory of Makes, AGORA, La Rivière, France
| | - J de Wit
- Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA, USA
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Morgado BE, Sicardy B, Braga-Ribas F, Ortiz JL, Salo H, Vachier F, Desmars J, Pereira CL, Santos-Sanz P, Sfair R, de Santana T, Assafin M, Vieira-Martins R, Gomes-Júnior AR, Margoti G, Dhillon VS, Fernández-Valenzuela E, Broughton J, Bradshaw J, Langersek R, Benedetti-Rossi G, Souami D, Holler BJ, Kretlow M, Boufleur RC, Camargo JIB, Duffard R, Beisker W, Morales N, Lecacheux J, Rommel FL, Herald D, Benz W, Jehin E, Jankowsky F, Marsh TR, Littlefair SP, Bruno G, Pagano I, Brandeker A, Collier-Cameron A, Florén HG, Hara N, Olofsson G, Wilson TG, Benkhaldoun Z, Busuttil R, Burdanov A, Ferrais M, Gault D, Gillon M, Hanna W, Kerr S, Kolb U, Nosworthy P, Sebastian D, Snodgrass C, Teng JP, de Wit J. A dense ring of the trans-Neptunian object Quaoar outside its Roche limit. Nature 2023; 614:239-243. [PMID: 36755175 DOI: 10.1038/s41586-022-05629-6] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/05/2022] [Accepted: 12/06/2022] [Indexed: 02/10/2023]
Abstract
Planetary rings are observed not only around giant planets1, but also around small bodies such as the Centaur Chariklo2 and the dwarf planet Haumea3. Up to now, all known dense rings were located close enough to their parent bodies, being inside the Roche limit, where tidal forces prevent material with reasonable densities from aggregating into a satellite. Here we report observations of an inhomogeneous ring around the trans-Neptunian body (50000) Quaoar. This trans-Neptunian object has an estimated radius4 of 555 km and possesses a roughly 80-km satellite5 (Weywot) that orbits at 24 Quaoar radii6,7. The detected ring orbits at 7.4 radii from the central body, which is well outside Quaoar's classical Roche limit, thus indicating that this limit does not always determine where ring material can survive. Our local collisional simulations show that elastic collisions, based on laboratory experiments8, can maintain a ring far away from the body. Moreover, Quaoar's ring orbits close to the 1/3 spin-orbit resonance9 with Quaoar, a property shared by Chariklo's2,10,11 and Haumea's3 rings, suggesting that this resonance plays a key role in ring confinement for small bodies.
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Affiliation(s)
- B E Morgado
- Federal University of Rio de Janeiro - Observatory of Valongo, Rio de Janeiro, Brazil.
- National Observatory/MCTI, Rio de Janeiro, Brazil.
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil.
| | - B Sicardy
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
| | - F Braga-Ribas
- Federal University of Technology, Paraná (UTFPR/DAFIS), Curitiba, Brazil
| | - J L Ortiz
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - H Salo
- Space Physics and Astronomy Research unit, University of Oulu, Oulu, Finland
| | - F Vachier
- The Institute of Celestial Mechanics and Ephemeris Calculation (IMCCE), Observatory of Paris, PSL Research University, CNRS, Sorbonne University, UPMC University of Paris, University of Lille, Lille, France
| | - J Desmars
- The Institute of Celestial Mechanics and Ephemeris Calculation (IMCCE), Observatory of Paris, PSL Research University, CNRS, Sorbonne University, UPMC University of Paris, University of Lille, Lille, France
- Polytechnic Institute of Advanced Sciences (IPSA), Ivry-sur-Seine, France
| | - C L Pereira
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - P Santos-Sanz
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - R Sfair
- Institute for Astronomy and Astrophysics, Eberhard Karls University of Tübingen, Tübingen, Germany
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - T de Santana
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - M Assafin
- Federal University of Rio de Janeiro - Observatory of Valongo, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - R Vieira-Martins
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - A R Gomes-Júnior
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
- Institute of Physics, Federal University of Uberlândia, Uberlândia, Brazil
| | - G Margoti
- Federal University of Technology, Paraná (UTFPR/DAFIS), Curitiba, Brazil
| | - V S Dhillon
- Department of Physics and Astronomy, University of Sheffield, Sheffield, UK
- Institute of Astrophysics of The Canary Islands, La Laguna, Spain
| | | | - J Broughton
- Reedy Creek Observatory, Gold Coast, Queensland, Australia
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - J Bradshaw
- Samford Valley Observatory (Q79), Brisbane, Queensland, Australia
| | - R Langersek
- Algester Astronomical Observatory, Brisbane, Queensland, Australia
| | - G Benedetti-Rossi
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
- Orbital Dynamics and Planetology Group, UNESP - São Paulo State University, Guaratinguetá, Brazil
| | - D Souami
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
- Observatory of the Côte d'Azur, Lagrange Laboratory UMR7293 CNRS, Nice, France
- naXys, University of Namur, Namur, Belgium
| | - B J Holler
- Space Telescope Science Institute, Baltimore, MD, USA
| | - M Kretlow
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
- International Occultation Timing Association / European Section, Hannover, Germany
- International Amateur Observatory e.V. (IAS), Mittenwalde, Germany
| | - R C Boufleur
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - J I B Camargo
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - R Duffard
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - W Beisker
- International Occultation Timing Association / European Section, Hannover, Germany
- International Amateur Observatory e.V. (IAS), Mittenwalde, Germany
| | - N Morales
- Institute of Astrophysics at Andalucía, IAA-CSIC, Granada, Spain
| | - J Lecacheux
- LESIA, Observatory of Paris, University PSL, CNRS, UPMC, Sorbonne University, University of Paris Diderot, Sorbonne Paris City, Meudon, France
| | - F L Rommel
- National Observatory/MCTI, Rio de Janeiro, Brazil
- Interinstitutional e-Astronomy Laboratory (LIneA), Rio de Janeiro, Brazil
| | - D Herald
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - W Benz
- Institute of Physics, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - E Jehin
- STAR Institute, University of Liège, Liège, Belgium
| | - F Jankowsky
- Heidelberg-Königstuhl State Observatory, Heidelberg, Germany
| | - T R Marsh
- Department of Physics, University of Warwick, Coventry, UK
| | - S P Littlefair
- Department of Physics and Astronomy, University of Sheffield, Sheffield, UK
| | - G Bruno
- INAF, Catania Astrophysical Observatory, Catania, Italy
| | - I Pagano
- INAF, Catania Astrophysical Observatory, Catania, Italy
| | - A Brandeker
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - A Collier-Cameron
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, UK
| | - H G Florén
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - N Hara
- Astronomical Observatory at the University of Geneva, Versoix, Switzerland
| | - G Olofsson
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - T G Wilson
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, UK
| | - Z Benkhaldoun
- Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Marrakech, Morocco
| | - R Busuttil
- School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, UK
| | - A Burdanov
- Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA, USA
| | - M Ferrais
- Laboratory of Astrophysics of Marseille, University of Aix Marseille, CNRS, CNES, Marseille, France
| | - D Gault
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - M Gillon
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | - W Hanna
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - S Kerr
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
- Astronomical Association of Queensland, Pimpama, Queensland, Australia
| | - U Kolb
- School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, UK
| | - P Nosworthy
- Trans-Tasman Occultation Alliance (TTOA), Wellington, New Zealand
| | - D Sebastian
- School of Physics and Astronomy, University of Birmingham, Birmingham, UK
| | - C Snodgrass
- Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK
| | - J P Teng
- AGORA Observatory of Makes, AGORA, La Rivière, France
| | - J de Wit
- Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA, USA
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Lebrun C, Vukusic S, Abadie V, Achour C, Ader F, Alchaar H, Alkhedr A, Andreux F, Androdias G, Arjmand R, Audoin B, Audry D, Aufauvre D, Autreaux C, Ayrignac X, Bailbe M, Benazet M, Bensa C, Bensmail D, Berger E, Bernady P, Bertagna Y, Biotti D, Blanchard-Dauphin A, Bonenfant J, Bonnan M, Bonnemain B, Borgel F, Botelho-Nevers E, Boucly S, Bourre B, Boutière C, Branger P, Brassat D, Bresch S, Breuil V, Brochet B, Brugeilles H, Bugnon P, Cabre P, Camdessanché JP, Carra-Dalière C, Casez O, Chamouard JM, Chassande B, Chataignier P, Chbicheb M, Chenet A, Ciron J, Clavelou P, Cohen M, Colamarino R, Collongues N, Coman I, Corail PR, Courtois S, Coustans M, Creange A, Creisson E, Daluzeau N, Davenas C, De Seze J, Debouverie M, Depaz R, Derache N, Divio L, Douay X, Dulau C, Durand-Dubief F, Edan G, Elias Z, Fagniez O, Faucher M, Faucheux JM, Fournier M, Gagneux-Brunon A, Gaida P, Galli P, Gallien P, Gaudelus J, Gault D, Gayou A, Genevray M, Gentil A, Gere J, Gignoux L, Giroux M, Givron P, Gout O, Grimaud J, Guennoc AM, Hadhoum N, Hautecoeur P, Heinzlef O, Jaeger M, Jeannin S, Kremer L, Kwiatkowski A, Labauge P, Labeyrie C, Lachaud S, Laffont I, Lanctin-Garcia C, Lannoy J, Lanotte L, Laplaud D, Latombe D, Lauxerois M, Le Page E, Lebrun-Frenay C, Lejeune P, Lejoyeux P, Lemonnier B, Leray E, Loche CM, Louapre C, Lubetzki C, Maarouf A, Mada B, Magy L, Maillart E, Manchon E, Marignier R, Marque P, Mathey G, Maurousset A, Mekies C, Merienne M, Michel L, Milor AM, Moisset X, Montcuquet A, Moreau T, Morel N, Moussa M, Naudillon JP, Normand M, Olive P, Ouallet JC, Outteryck O, Pacault C, Papeix C, Patry I, Peaureaux D, Pelletier J, Pichon B, Pittion S, Planque E, Pouget MC, Pourcher V, Radot C, Robert I, Rocher F, Ruet A, Ruet A, Saint-Val C, Salle JY, Salmon A, Sartori E, Schaeffer S, Stankhof B, Taithe F, Thouvenot E, Tizon C, Tourbah A, Tourniaire P, Vaillant M, Vermersch P, Vidil S, Wahab A, Warter MH, Wiertlewski S, Wiplosz B, Wittwer B, Zaenker C, Zephir H. Immunization and multiple sclerosis: Recommendations from the French Multiple Sclerosis Society. Rev Neurol (Paris) 2019; 175:341-357. [DOI: 10.1016/j.neurol.2019.04.001] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/30/2019] [Revised: 03/31/2019] [Accepted: 04/11/2019] [Indexed: 10/26/2022]
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Fattal C, Albert T, Le-Chapelain L, Gault D, Goossens D, Perrouin-Verbe B. A recent survey relating to the organization of the French network of spinal cord injuries care units. Ann Phys Rehabil Med 2018. [DOI: 10.1016/j.rehab.2018.05.1183] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/28/2022]
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Gelis A, Daures JP, Gault D, Bouchema T, Pedelucq JP, Maupas E, Goossens D, Pelissier J, Fattal C. Auto-évaluation des mesures de prévention cutanées chez les personnes lésées médullaires : validation de la version française du SMnac. Ann Phys Rehabil Med 2012. [DOI: 10.1016/j.rehab.2012.07.348] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
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Gelis A, Daures JP, Gault D, Bouchema T, Pedelucq JP, Maupas E, Goossens D, Pelissier J, Fattal C. Evaluating self-reported pressure ulcer prevention measures in person with spinal cord injury using the SMnac: Validation of the French version. Ann Phys Rehabil Med 2012. [DOI: 10.1016/j.rehab.2012.07.354] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Marsh D, Sabbagh W, Gault D. Cryptotia correction – the post-auricular transposition flap. J Plast Reconstr Aesthet Surg 2011; 64:1444-7. [DOI: 10.1016/j.bjps.2011.06.037] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/23/2011] [Revised: 03/30/2011] [Accepted: 06/24/2011] [Indexed: 11/26/2022]
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Gélis A, Stéfan A, Colin D, Albert T, Gault D, Goossens D, Perrouin-Verbe B, Fattal C, Pelissier J, Coudeyre E. Therapeutic education in persons with spinal cord injury: A review of the literature. Ann Phys Rehabil Med 2011; 54:189-210. [DOI: 10.1016/j.rehab.2011.03.004] [Citation(s) in RCA: 27] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/20/2010] [Revised: 03/13/2011] [Accepted: 03/17/2011] [Indexed: 11/24/2022]
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Gault D, Morel-Fatio M, Albert T, Fattal C. Chronic neuropathic pain of spinal cord injury: What is the effectiveness of psychocomportemental management? Ann Phys Rehabil Med 2009; 52:167-72. [DOI: 10.1016/j.rehab.2008.12.007] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/15/2008] [Accepted: 12/17/2008] [Indexed: 11/29/2022]
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Bajaj Y, Wyatt ME, Gault D, Bailey CM, Albert DM. How we do it: BAHA positioning in patients with microtia requiring auricular reconstruction. Clin Otolaryngol 2005; 30:468-71. [PMID: 16232256 DOI: 10.1111/j.1365-2273.2005.01041.x] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/29/2022]
Abstract
Keypoints * Bilateral microtia is a challenging problem as these patients require both reconstruction of the auricle and rehabilitation of hearing. * Our aim was to find the optimal position for bone-anchored hearing aids (BAHA) in patients requiring reconstruction of the auricle on the same side. * From an analysis of five such operated patients, it was found that siting a BAHA 6.5-7.0 cm from the position of the external auditory meatus is probably the correct distance to facilitate optimal auricular reconstruction. * Using these criteria, a group of another five patients with BAHA awaiting auricular reconstruction were reviewed. Of these only three (60%) have been satisfactorily sited.
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11
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Townley WA, Durrant CAT, Gault D. Mastectomy and reconstruction--an unusual solution to intractable breast pain. Breast 2004; 13:359-61. [PMID: 15325676 DOI: 10.1016/j.breast.2004.01.002] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/18/2003] [Revised: 12/19/2003] [Accepted: 01/07/2004] [Indexed: 11/25/2022] Open
Abstract
Breast pain is a common complaint which usually subsides with simple reassurance or sometimes medication. This paper describes the case of a 41-year-old woman suffering from severe non-cyclical breast pain that had proved resistant to a battery of medical treatments. The pain was so disabling that it drove the patient to contemplate suicide. At the patient's request, a bilateral subcutaneous mastectomy with immediate implant reconstruction was performed, resulting in a complete resolution of the pain. Non-cyclical breast pain is less common than cyclical breast pain and tends to be more difficult to treat. This case suggests that mastectomy may be an appropriate option of last resort in the treatment of severe intractable breast pain.
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Affiliation(s)
- W A Townley
- Department of Plastic Surgery, Mount Vernon Hospital, Northwood, UK.
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12
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Rimmer J, Hamilton S, Gault D. Recurrent mycobacterial breast abscesses complicating reconstruction. ACTA ACUST UNITED AC 2004; 57:676-8. [PMID: 15380702 DOI: 10.1016/j.bjps.2004.06.015] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/11/2003] [Accepted: 06/11/2004] [Indexed: 10/26/2022]
Abstract
We present a patient with mycobacterial infection of the breast and subsequent mastectomy. After initial reconstruction, she developed multiple recurrent abscesses around the flap. This necessitated further debridement and a second reconstruction. This case demonstrates the need to beware mycobacterial infection in patients undergoing breast reconstruction, especially after recurrent "sterile" abscesses.
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Affiliation(s)
- J Rimmer
- Plastic Surgery Unit, Mount Vernon Hospital, Rickmansworth Road, Northwood HA6 2JR, UK
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13
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Abstract
Whilst tuberous female breasts are well described, the tuberous male breast is a very unusual variant of gynaecomastia. Two cases are presented, the development of the condition is considered and the surgical management is discussed.
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Affiliation(s)
- S Hamilton
- Department of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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14
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15
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Topping A, Gault D, Grobbelaar A, Sanders R, Green C, Linge C. Does low penetration of human skin by the normal mode ruby laser account for poor permanent depilatory success rates? Lasers Med Sci 2002; 16:224-9. [PMID: 11482822 DOI: 10.1007/pl00011359] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/25/2022]
Abstract
Studies reported to date have shown a good depilatory response from patients treated with the normal mode ruby laser (NMRL) over 12 weeks, but a low response over a time period greater than this. Previous publications have suggested that this could be accounted for by the apparently poor skin penetration of laser light and so this study attempted to assess whether this was indeed the case. Skin samples of varying thicknesses were taken from six Caucasian patients and their depths measured. Each was laid individually on an energy meter before having pulses from an NMRL compatible with clinical doses (4.75 J/cm2, 9.24 J/cm2 and 13.41 J/cm2) fired on the epidermis. Several samples had the laser fired repetitively on the surface to assess whether this caused any change in laser/skin fluence depth profiles. Repetitive firing of the NMRL on the epidermis of skin samples did not alter the energy recorded by the meter beneath. The fluence/depth profiles were constructed showing the majority of energy was lost within the first 1 mm of the skin surface (50%) which then further reduced over distance but at a much slower rate. The maximum depth of penetration was 14.8 mm (SD +/- 0.478) which appeared to be a function of wavelength and not fluence. The results suggest that laser penetration of skin should be adequate for generating enough heat at the hair bulge and bulb, potentially causing permanent damage. The implications of this study are that it is probably the presence of the correct chromophore in large enough amounts which is required for successful permanent depilation to occur.
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Affiliation(s)
- A Topping
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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16
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Abstract
An auricular keloid occurring following ear-piercing remains a difficult condition to treat. Various treatments have been described, with different reported degrees of success. Pressure therapy has been shown to be an effective treatment for auricular keloids, although the devices used have not all been universally accepted. We assessed 30 patients, between 1989 and 1999, who had been fitted with pressure devices made from Zimmer splints. There was a 50% or greater reduction in the size of each keloid when assessed at 1 year. Zimmer splints are cheap, readily available, easily moulded to fit the patient and can be decorated so that they can be worn as earrings.
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Affiliation(s)
- R Russell
- Plastic Surgery Unit, Mount Vernon Hospital, Northwood, UK
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17
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Botma M, Aymat A, Gault D, Albert DM. Rib graft reconstruction versus osseointegrated prosthesis for microtia: a significant change in patient preference. Clin Otolaryngol Allied Sci 2001; 26:274-7. [PMID: 11559335 DOI: 10.1046/j.1365-2273.2001.00454.x] [Citation(s) in RCA: 15] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
Until recently the options for reconstruction of the microtic ear were unsatisfactory and the ear was often left alone. With recent advances, both autologous rib reconstruction and osseointegration produce good quality results. It is our practice to offer all patients a choice of no surgery, autologous rib cartilage reconstruction or an osseointegrated prosthetic ear. This study reports on parental choice between the reconstructive options as assessed by questionnaire. Earlier patients who have had their surgery were compared with more recent patients who have chosen an option but are awaiting surgery. In the patients who have had surgery, seven (30%) chose a prosthetic ear and 16 (69.5%) chose rib cartilage reconstruction, compared to those patients that are awaiting surgery, four (11%) chose a prosthetic ear and 31 (88.6%) chose rib cartilage reconstruction. The results show a significant increase in the choice for rib cartilage reconstruction in those patients awaiting surgery. Although high quality autologous reconstruction is not widely available we feel it is important that parents are at least informed that it is an alternative to osseointegration and no surgery.
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Affiliation(s)
- M Botma
- Great Ormond Street Hospital, London, UK.
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18
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Affiliation(s)
- D. Gault
- Mount Vernon Hospital Rickmansworth Road Northwood, Middlesex, HA6 2RN
| | - B. Jemec
- Mount Vernon Hospital Rickmansworth Road Northwood, Middlesex, HA6 2RN
| | - S. Cicchetti
- Mount Vernon Hospital Rickmansworth Road Northwood, Middlesex, HA6 2RN
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19
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Topping A, Gault D, Grobbelaar A, Green C, Sanders R, Sibbons P, Linge C. Successful reduction in skin damage resulting from exposure to the normal-mode ruby laser in an animal model. Br J Plast Surg 2001; 54:144-50. [PMID: 11207126 DOI: 10.1054/bjps.2000.3501] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/18/2022]
Abstract
Normal-mode ruby laser (NMRL) irradiation of skin has now become an acceptable method of producing depilation. However, side effects, which include superficial burning and changes in skin pigmentation, still occur and, although temporary, can be distressing to the patient. This paper reports a method by which the skin can be protected (or preconditioned) from damage during NMRL treatment by pre-heating to a lower, non-damaging level prior to irradiation. Using the black-haired mouse (C57B1/10) as an animal model, an appropriate 'preconditioning' temperature was established by exposing the mouse skin to a range of temperatures, taking biopsies and staining the skin immunohistochemically for heat shock protein 70 (HSP 70) expression within the keratinocyte cells. Increased HSP 70 expression is stimulated by exposure to environmental stressors such as heat, so it was hypothesised that its increased expression conveyed increased cellular protection. The appropriate temperature (45 degrees C for 15 min) allowed for the superficial skin cells to be protected (as assessed by maximal HSP 70 staining) but undamaged (as assessed by haematoxylin and eosin staining), leaving the target hair-producing cells unprotected. Eight mice (16 flanks) were then exposed to this preconditioning temperature (eight of the flanks being growing-hair sites and eight resting-hair sites) and 5 h later exposed to a laser fluence known to cause mild skin damage and depilation (6J/cm2). This exposure was to both the preconditioned and the adjacent non-preconditioned sites. A statistically significant reduction in skin damage (P <0.001), as measured by the time taken to heal and noted both clinically and histologically, was seen in the preconditioned sites in resting-hair regions but not in growing-hair regions. Depilation, established over an 8 week period, was successful in growing-hair regions within both preconditioned and non-preconditioned sites, but complete hair regrowth had occurred in preconditioned and non-preconditioned sites within resting-hair regions by 5 weeks. The latter finding was consistent with work already reported suggesting that NMRL-assisted depilation in this animal model is not successful for hairs in the telogen phase. Successful preconditioning of mouse skin prior to laser exposure appears to reduce NMRL-induced skin side effects. In addition, the technique does not appear to adversely affect successful depilation.
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Affiliation(s)
- A Topping
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, UK
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20
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Abstract
OBJECTIVE The purpose of this study was to assess the efficacy of laser assisted hair removal in children aged 16 and under using the long pulsed ruby laser. BACKGROUND DATA Unwanted hair in the pediatric population can be due to congenital hairy nevi and hypertrichosis. Methods of effecting hair removal include shaving, electrolysis, and laser depilation. The long-pulsed ruby laser is an established treatment modality in adults, but its use specifically in children has not been investigated. METHODS Patients aged 16 or under undergoing treatment with the ruby laser for unwanted hair were assessed. Hair counts were determined before and after treatment and an assessment of overall satisfaction was made using a parental questionnaire. RESULTS Treatment was regarded as successful in 25 out of 28 cases where there was a clear reduction in hair growth at the site treated with an average fall in hair count of 63% at 6 months follow up. There was no scarring or hyperpigmentation in this group and no serious complications. Total suppression of hair growth was not permanent but usually lasted between 3 and 6 months. Few problems were encountered from using the technique specifically in children, and pain was well controlled in most cases. CONCLUSIONS We would recommend the long-pulsed ruby laser as a useful form of hair removal in children that is quick, simple and well tolerated. At present, the technique leads to hair loss that is temporary but most patients and their parents feel the treatment gives worthwhile benefits.
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Affiliation(s)
- S Morley
- Department of Plastic Surgery, Restoration of Appearance and Function Trust, Mount Vernon Hospital, Northwood, Middlesex, UK.
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21
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22
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Sylaidis P, Gault D. Antihelical folding for pinnaplasty using one posterior cartilage score and horizontal mattress sutures. Ann Plast Surg 2000; 45:341-3. [PMID: 10987544] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/17/2023]
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23
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Topping A, Gault D, Grobbelaar A, Green C, Sanders R, Linge C. The temperatures reached and the damage caused to hair follicles by the normal-mode ruby laser when used for depilation. Ann Plast Surg 2000; 44:581-90. [PMID: 10884072 DOI: 10.1097/00000637-200044060-00001] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
Abstract
Although it is proposed that heat is the cause of follicular damage leading to depilation, this has never been proved. This study aims to determine the mode by which depilation is effected and, if heat is the mechanism, what temperatures are reached within treated follicles and if sufficient damage is produced therein. Two excised specimens of hair-bearing skin from 5 patients undergoing facelifts were dissected to reveal the hair bulbs/shafts on the deep surface. They were placed on a jig, and one pulse from a normal-mode ruby laser (NMRL) of 15 J per square centimeter was fired on the epidermal surface. A thermal imaging camera recorded dermal temperature changes on the deep surface in real time. Specimens were then examined histologically for the site and extent of cellular damage by immunohistochemical staining for a protein marker of cell damage (p53). The NMRL targeted hair follicles specifically. The most common follicular temperature increase ranged from 5 to 10 degrees C. In specimens from 1 patient the increase was more than 30 degrees C (p < 0.001). Heat dissipation into interfollicular tissue in all specimens occurred 2 seconds after exposure. Evidence of laser-induced damage to follicle-lining cells was found only in those follicles with damaged hair shafts. The changes were found to a greater depth (to the bulb) and greater extent (beyond the bulge) in those follicles reaching higher temperatures. These findings suggest that the NMRL should produce permanent depilation. The variability between follicles and between patients explains, perhaps, the uneven outcome regarding depilation using the NMRL. Success appears to depend on peak follicular temperatures achieved during laser exposure, which may result from the follicular characteristics of the individual patient.
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Affiliation(s)
- A Topping
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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24
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Abstract
There is a clinical need in the fields of reconstructive and cosmetic plastic surgery for a safe, simple, and effective method of hair depilation. Depilatory clinics have been established throughout the country, commonly using the ruby laser, to treat a cohort of the population, estimated to be between 6% and 10%, recognized as being hirsute. Clinical trials performed to date have not established a protocol that suits the previously mentioned criteria and have been, usually, small in number and short in follow-up. With the increased use that this form of laser treatment will inevitably undergo, it is the belief of the authors that the only way of ascertaining whether the treatment is safe, simple, and effective is first to establish how the ruby laser works. This review relates the knowledge that is currently available regarding the function of the ruby laser to a number of the clinical studies that have been undertaken, including three that have used other types of laser. Using this information, future areas in which research is required can be defined, ultimately to improve the clinical efficacy of ruby laser-assisted hair removal while lessening the current side effects (namely, superficial burning, and hypo- and hyperpigmentation).
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Affiliation(s)
- A Topping
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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25
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Abstract
A modification to a standard nasolabial flap is described for the simultaneous reconstruction of confluent perialar and full thickness alar defects. The main body of the flap is advanced to cover the external surface of the perialar and alar defects. A side extension to the flap, based only on a dermal blood supply, is turned over, to line the reconstructed alar rim.
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Affiliation(s)
- D L Feinendegen
- Department of Plastic and Reconstructive Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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26
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Liew SH, Grobbelaar A, Gault D, Sanders R, Green C, Linge C. Hair removal using the ruby laser: clinical efficacy in Fitzpatrick skin types I-V and histological changes in epidermal melanocytes. Br J Dermatol 1999; 140:1105-9. [PMID: 10354078 DOI: 10.1046/j.1365-2133.1999.02911.x] [Citation(s) in RCA: 34] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
The ruby laser is effective in removing unwanted body hair. The occurrence of cutaneous side-effects such as blistering, hypopigmentation and hyperpigmentation, however, remains problematic. These side-effects are more commonly seen in patients with dark coloured skin, which partly explains the relative scarcity of information on the efficacy of ruby laser hair removal in such patients. The mechanisms of the occurrence of these side-effects are also not known. It was the aim of this study to evaluate the efficacy of ruby laser-assisted hair removal in patients with Fitzpatrick skin type V in a retrospective clinical study and to evaluate the mechanism of post-treatment pigmentary change in a prospective clinical study. The percentage reduction in hair density in patients with skin type V was assessed after a variable period following treatment with the Chromos 694 Depilation Ruby Laser, and was compared with the results of those with skin types I-IV. To study the pigmentary change and melanocyte numbers after laser irradiation, ex-vivo scalp skin and serial patient biopsies were taken and stained with S-100, dopa oxidase and Masson-Fontana methods. Laser treatment reduced melanocyte numbers as measured by DOPA stain but not by S100. Laser treatment resulted in the clearance of pigment from the epidermis on histology. Ruby laser was shown to be effective in removing unwanted hair from patients with dark coloured skin, but with a higher incidence of cutaneous side-effects. The occurrence of hypopigmentation after laser irradiation was thought to be due to the suppression of melanogenesis in the epidermis rather than to destruction of the melanocytes.
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Affiliation(s)
- S H Liew
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex HA6 2RN, U.K
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27
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28
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Kelly MB, Bosmans L, Gault D. Use of the palmaris brevis flap for preventing recurrent median nerve compression in mucolipidosis. J Hand Surg Br 1999; 24:300-2. [PMID: 10433441 DOI: 10.1054/jhsb.1999.0064] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/18/2022]
Abstract
In a patient with severe, recurrent bilateral carpal tunnel syndrome secondary to mucolipidosis, the 'turnover' palmaris brevis flap was used in conjunction with internal neurolysis. The procedure was effective in alleviating symptoms of recurrent carpal tunnel compression in both hands.
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Affiliation(s)
- M B Kelly
- Department of Plastic and Reconstructive Surgery, Mount Vernon Hospital, Northwood, UK.
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29
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Sommerlad BC, Gault D. Space-obliterating skin suture. Plast Reconstr Surg 1999; 103:1101. [PMID: 10077135] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/11/2023]
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30
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Liew SH, Grobbelaar AO, Gault D, Green C, Linge C. Ruby laser-assisted hair removal: a preliminary report of the correlation between efficacy of treatment and melanin content of hair and the growth phases of hair at a specific site. Ann Plast Surg 1999; 42:255-8. [PMID: 10096615 DOI: 10.1097/00000637-199903000-00005] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
Abstract
An unpredictable response, even in patients with dark hair, often undermines successful ruby laser hair removal. A prospective clinical study was carried out to evaluate the roles of melanin content and growth phases of hair in treatment efficacy. Thirty-six volunteers with white skin and dark hair were recruited for the study, and were all treated using the Chromos 694 Depilation Ruby Laser. The overall efficacy of treatment was assessed at the end of 3 months. The efficacy of laser treatment is not due solely to the proportion of hair in the growing or static phase of the hair cycle. There is a lack of correlation between the melanin content and the overall efficacy of laser hair removal in those treated once, but patients with darker hair responded better after repeated treatments. The proportion of hair in the growth phase and the melanin content of hair do not contribute solely to the efficacy of ruby laser hair removal.
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Affiliation(s)
- S H Liew
- RAFT Institute of Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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31
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32
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Abstract
A case is reported of length discrepancy between the two thumbs in a 12-year-old girl following trauma to her left thumb twice before the age of 3 years. The distal phalanx of the left thumb overgrew by 5 mm. There was no functional disability and surgery was requested to improve the appearance.
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Affiliation(s)
- M M Shibu
- Plastic Surgery Department, Mount Vernon Hospital, Northwood, Middlesex, UK
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33
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Gault D. Invited commentary. Eur J Plast Surg 1995. [DOI: 10.1007/bf00178543] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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34
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Abstract
There is a high incidence of postoperative nausea and vomiting after surgical correction of prominent ears. A prospective, randomized study was performed to determine if the method of dressing the ears influenced the incidence of postoperative vomiting. Avoidance of packing the external auditory meatus and concha produced a significant reduction in postoperative nausea (83% vs 30%; P < 0.005) and vomiting (63% vs 22%; P < 0.01).
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Affiliation(s)
- P Ridings
- RAFT Department of Research in Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex
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35
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Abstract
Compartment syndrome in the upper arm is uncommon, but early recognition and treatment is as essential as it is in other sites. A case of compartment syndrome in the upper arm is reported.
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Affiliation(s)
- P Ridings
- RAFT Department of Research in Plastic Surgery, Mount Vernon Hospital, Northwood, Middlesex, UK
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36
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Abstract
Two cases are reported of serious extravasation injuries due to parenteral nutrition in infants born at 24 and 28 weeks' gestation. Major scarring and the need for plastic surgery were prevented by using a technique of subcutaneous hyaluronidase and saline flushing.
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Affiliation(s)
- J Davies
- Department of Paediatrics, Hillingdon Hospital, Uxbridge, Middlesex
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37
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38
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39
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Gault D, Sommerlad B. Suturing skin under tension. Plast Reconstr Surg 1989; 83:391. [PMID: 2643130 DOI: 10.1097/00006534-198902000-00047] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/01/2023]
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40
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Abstract
A method of calculating intracranial volume from horizontal computerized tomography scan slices is presented. The accuracy of this technique was confirmed by applying it to 10 dry skulls and comparing the values obtained with the true intracranial volumes, as determined by filling the skulls with water. Values ranging between 98.14% and 102.6% of the true values were obtained, the mean error being 1.13%. This technique is now being used to study intracranial volume changes in children with craniostenosis.
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Affiliation(s)
- D Gault
- Centre for Craniofacial Anomalies, Hospital Necker-Enfants Malades, Paris, France
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41
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Gault D, McGeorge D. The image of plastic surgery. Practitioner 1988; 232:709-11. [PMID: 3249734] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/04/2023]
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42
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Gault D. The use of pre-printed hand assessment charts. J Hand Surg Br 1987. [PMID: 3624999 DOI: 10.1016/0266-7681(87)90036-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 01/06/2023]
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43
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Gault D. Letter to the Editor. Journal of Hand Surgery 1987; 12:285. [PMID: 3624999 DOI: 10.1016/0266-7681_87_90036-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 10/19/2022]
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44
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Elliot D, Everitt AS, Gault D, Quaba AA, Hackett ME, Howlett TA, Tomlin SJ, Rees LH. The role of endorphins in septicaemic shock: a pilot study in burned patients. Burns 1985; 11:387-92. [PMID: 2931160 DOI: 10.1016/0305-4179(85)90142-1] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/03/2023]
Abstract
There is recent evidence that circulating opioid peptides, or 'endorphins', act as chemical messengers responsible for the induction of the complex cardiovascular changes leading to hypotension in septicaemic shock. The pilot study of an investigation of opioid peptides in septicaemia in burned patients is presented. Serial measurements of plasma beta-endorphin and metenkephalin were performed throughout the recovery of six patients with large burns (20-70 per cent BSA). Our preliminary findings concur with previous evidence that opioid peptides may play a role in the hypotension of septicaemic shock.
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45
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Adiseshiah M, Gault D. Exteriorisation resection of the colon. Ann R Coll Surg Engl 1982; 64:321-3. [PMID: 7114767 PMCID: PMC2494111] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/23/2023] Open
Abstract
The early results of 34 exteriorisation resections of the colon are presented, 25 being emergency procedures and 9 elective. The operative mortality in the emergency group was 20% and there were no deaths in the elective group. All patients who survived the postoperative period have had their colostomies closed. The operation was technically simple and quick to perform. It is one of the safest methods of resecting colon. The technique proved to be a useful alternative to standard techniques in colonic perforation, colonic obstruction with proximal faecal retention, nonviable sigmoid volvulus, diverticular disease requiring resection, and colovesical and colouterine fistula.
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46
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Murray BC, Belton MJ, Danielson GE, Davies ME, Gault D, Hapke B, O'leary B, Strom RG, Suomi V, Trask N. Mariner 10 Pictures of Mercury: First Results. Science 1974; 184:459-61. [PMID: 17736516 DOI: 10.1126/science.184.4135.459] [Citation(s) in RCA: 17] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Mercury has a heavily cratered surface cotntaining basins up to at least 1300 kilometers diameter flooded with mare-like material. Many features are closely similar to those on the moon, but significant structural differences exist. Major chemical differentiation before termination of accretion is implied.
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Murray BC, Belton MJ, Danielson GE, Davies ME, Gault D, Hapke B, O'leary B, Strom RG, Suomi V, Trask N. Venus: Atmospheric Motion and Structure from Mariner 10 Pictures. Science 1974; 183:1307-15. [PMID: 17791373 DOI: 10.1126/science.183.4131.1307] [Citation(s) in RCA: 99] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Mariner 10 television camieras imaged the planet Venus in the visible and near ultraviolet for a period of 8 days at resolutions ranging from 100 meters to 130 kilometers. Tle general pattern of the atmospheric circulation in the upper tropospheric/lower stratospheric region is displayed in the pictures. Atmospheric flow is symmetrical between north and south hemispheres. The equatorial motions are zonal (east-west) at approxiimnately 100 meters per second, consistent with the previously inferred 4-day retrograde rotation. Angular velocity increases with latitude. The subsolar region, and the region downwind from it, show evidence of large-scale convection that persists in spite of the main zonal motion. Dynamical interaction between the zonal motion and the relatively stationary region of convection is evidenced by bowlike waves.
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