1
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Zimmerman EA, Irani I, Chen P, Gal-Yam A, Schulze S, Perley DA, Sollerman J, Filippenko AV, Shenar T, Yaron O, Shahaf S, Bruch RJ, Ofek EO, De Cia A, Brink TG, Yang Y, Vasylyev SS, Ben Ami S, Aubert M, Badash A, Bloom JS, Brown PJ, De K, Dimitriadis G, Fransson C, Fremling C, Hinds K, Horesh A, Johansson JP, Kasliwal MM, Kulkarni SR, Kushnir D, Martin C, Matuzewski M, McGurk RC, Miller AA, Morag J, Neil JD, Nugent PE, Post RS, Prusinski NZ, Qin Y, Raichoor A, Riddle R, Rowe M, Rusholme B, Sfaradi I, Sjoberg KM, Soumagnac M, Stein RD, Strotjohann NL, Terwel JH, Wasserman T, Wise J, Wold A, Yan L, Zhang K. The complex circumstellar environment of supernova 2023ixf. Nature 2024; 627:759-762. [PMID: 38538936 DOI: 10.1038/s41586-024-07116-6] [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: 10/03/2023] [Accepted: 01/24/2024] [Indexed: 04/01/2024]
Abstract
The early evolution of a supernova (SN) can reveal information about the environment and the progenitor star. When a star explodes in vacuum, the first photons to escape from its surface appear as a brief, hours-long shock-breakout flare1,2, followed by a cooling phase of emission. However, for stars exploding within a distribution of dense, optically thick circumstellar material (CSM), the first photons escape from the material beyond the stellar edge and the duration of the initial flare can extend to several days, during which the escaping emission indicates photospheric heating3. Early serendipitous observations2,4 that lacked ultraviolet (UV) data were unable to determine whether the early emission is heating or cooling and hence the nature of the early explosion event. Here we report UV spectra of the nearby SN 2023ixf in the galaxy Messier 101 (M101). Using the UV data as well as a comprehensive set of further multiwavelength observations, we temporally resolve the emergence of the explosion shock from a thick medium heated by the SN emission. We derive a reliable bolometric light curve that indicates that the shock breaks out from a dense layer with a radius substantially larger than typical supergiants.
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Affiliation(s)
- E A Zimmerman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel.
| | - I Irani
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - P Chen
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - A Gal-Yam
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - S Schulze
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, Sweden
| | - D A Perley
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
| | - J Sollerman
- The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden
| | - A V Filippenko
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - T Shenar
- Departamento de Astrofísica, Centro de Astrobiología (CSIC-INTA), Madrid, Spain
| | - O Yaron
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - S Shahaf
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - R J Bruch
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
- School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel
| | - E O Ofek
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - A De Cia
- European Southern Observatory, Garching bei München, Germany
- Department of Astronomy, University of Geneva, Versoix, Switzerland
| | - T G Brink
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - Y Yang
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
- Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing, China
| | - S S Vasylyev
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - S Ben Ami
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - M Aubert
- Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France
| | - A Badash
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - J S Bloom
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - P J Brown
- Department of Physics and Astronomy, Texas A&M University, College Station, TX, USA
| | - K De
- MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA, USA
| | - G Dimitriadis
- School of Physics, Trinity College Dublin, The University of Dublin, Dublin 2, Ireland
| | - C Fransson
- The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden
| | - C Fremling
- Caltech Optical Observatories, California Institute of Technology, Pasadena, CA, USA
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - K Hinds
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
| | - A Horesh
- The Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, Israel
| | - J P Johansson
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, Sweden
| | - M M Kasliwal
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - S R Kulkarni
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - D Kushnir
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - C Martin
- Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA, USA
| | - M Matuzewski
- Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA, USA
| | - R C McGurk
- W. M. Keck Observatory, Kamuela, HI, USA
| | - A A Miller
- Department of Physics and Astronomy, Northwestern University, Evanston, IL, USA
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University, Evanston, IL, USA
| | - J Morag
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - J D Neil
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - P E Nugent
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
- Lawrence Berkeley National Laboratory, Berkeley, CA, USA
| | - R S Post
- Post Observatory, Lexington, MA, USA
| | - N Z Prusinski
- Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA, USA
| | - Y Qin
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - A Raichoor
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - R Riddle
- Caltech Optical Observatories, California Institute of Technology, Pasadena, CA, USA
| | - M Rowe
- Department of Physics and Astronomy, Texas A&M University, College Station, TX, USA
| | - B Rusholme
- IPAC, California Institute of Technology, Pasadena, CA, USA
| | - I Sfaradi
- The Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, Israel
| | - K M Sjoberg
- Department of Astronomy, Harvard University, Cambridge, MA, USA
- Isaac Newton Group (ING), Santa Cruz de La Palma, Canary Islands, Spain
| | - M Soumagnac
- Lawrence Berkeley National Laboratory, Berkeley, CA, USA
- Department of Physics, Bar-Ilan University, Ramat Gan, Israel
| | - R D Stein
- Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - N L Strotjohann
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - J H Terwel
- School of Physics, Trinity College Dublin, The University of Dublin, Dublin 2, Ireland
- Isaac Newton Group (ING), Santa Cruz de La Palma, Canary Islands, Spain
| | - T Wasserman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - J Wise
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
| | - A Wold
- IPAC, California Institute of Technology, Pasadena, CA, USA
| | - L Yan
- Caltech Optical Observatories, California Institute of Technology, Pasadena, CA, USA
| | - K Zhang
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
- Department of Astronomy & Astrophysics, University of California, San Diego, La Jolla, CA, USA
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2
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Gal-Yam A, Bruch R, Schulze S, Yang Y, Perley DA, Irani I, Sollerman J, Kool EC, Soumagnac MT, Yaron O, Strotjohann NL, Zimmerman E, Barbarino C, Kulkarni SR, Kasliwal MM, De K, Yao Y, Fremling C, Yan L, Ofek EO, Fransson C, Filippenko AV, Zheng W, Brink TG, Copperwheat CM, Foley RJ, Brown J, Siebert M, Leloudas G, Cabrera-Lavers AL, Garcia-Alvarez D, Marante-Barreto A, Frederick S, Hung T, Wheeler JC, Vinkó J, Thomas BP, Graham MJ, Duev DA, Drake AJ, Dekany R, Bellm EC, Rusholme B, Shupe DL, Andreoni I, Sharma Y, Riddle R, van Roestel J, Knezevic N. A WC/WO star exploding within an expanding carbon-oxygen-neon nebula. Nature 2022; 601:201-204. [PMID: 35022591 DOI: 10.1038/s41586-021-04155-1] [Citation(s) in RCA: 17] [Impact Index Per Article: 8.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/06/2021] [Accepted: 10/15/2021] [Indexed: 11/09/2022]
Abstract
The final fate of massive stars, and the nature of the compact remnants they leave behind (black holes and neutron stars), are open questions in astrophysics. Many massive stars are stripped of their outer hydrogen envelopes as they evolve. Such Wolf-Rayet stars1 emit strong and rapidly expanding winds with speeds greater than 1,000 kilometres per second. A fraction of this population is also helium-depleted, with spectra dominated by highly ionized emission lines of carbon and oxygen (types WC/WO). Evidence indicates that the most commonly observed supernova explosions that lack hydrogen and helium (types Ib/Ic) cannot result from massive WC/WO stars2,3, leading some to suggest that most such stars collapse directly into black holes without a visible supernova explosion4. Here we report observations of SN 2019hgp, beginning about a day after the explosion. Its short rise time and rapid decline place it among an emerging population of rapidly evolving transients5-8. Spectroscopy reveals a rich set of emission lines indicating that the explosion occurred within a nebula composed of carbon, oxygen and neon. Narrow absorption features show that this material is expanding at high velocities (greater than 1,500 kilometres per second), requiring a compact progenitor. Our observations are consistent with an explosion of a massive WC/WO star, and suggest that massive Wolf-Rayet stars may be the progenitors of some rapidly evolving transients.
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Affiliation(s)
- A Gal-Yam
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel.
| | - R Bruch
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - S Schulze
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel.,The Oskar Klein Centre, Department of Astronomy and Department of Physics, AlbaNova, Stockholm University, Stockholm, Sweden
| | - Y Yang
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel.,Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - D A Perley
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
| | - I Irani
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - J Sollerman
- The Oskar Klein Centre, Department of Astronomy and Department of Physics, AlbaNova, Stockholm University, Stockholm, Sweden
| | - E C Kool
- The Oskar Klein Centre, Department of Astronomy and Department of Physics, AlbaNova, Stockholm University, Stockholm, Sweden
| | - M T Soumagnac
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel.,Lawrence Berkeley National Laboratory, Berkeley, CA, USA
| | - O Yaron
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - N L Strotjohann
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - E Zimmerman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - C Barbarino
- The Oskar Klein Centre, Department of Astronomy and Department of Physics, AlbaNova, Stockholm University, Stockholm, Sweden
| | - S R Kulkarni
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - M M Kasliwal
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - K De
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - Y Yao
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - C Fremling
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - L Yan
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - E O Ofek
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
| | - C Fransson
- The Oskar Klein Centre, Department of Astronomy and Department of Physics, AlbaNova, Stockholm University, Stockholm, Sweden
| | - A V Filippenko
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA.,Miller Institute for Basic Research in Science, University of California, Berkeley, Berkeley, CA, USA
| | - W Zheng
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - T G Brink
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - C M Copperwheat
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
| | - R J Foley
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - J Brown
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - M Siebert
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - G Leloudas
- DTU Space, National Space Institute, Technical University of Denmark, Kongens Lyngby, Denmark
| | | | | | | | - S Frederick
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - T Hung
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - J C Wheeler
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA
| | - J Vinkó
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA.,Konkoly Observatory, ELKH CSFK, Budapest, Hungary.,Department of Optics and Quantum Electronics, University of Szeged, Szeged, Hungary.,ELTE Institute of Physics, Eötvös Loránd University, Budapest, Hungary
| | - B P Thomas
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA
| | - M J Graham
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - D A Duev
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - A J Drake
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - R Dekany
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - E C Bellm
- DIRAC Institute, Department of Astronomy, University of Washington, Seattle, WA, USA
| | - B Rusholme
- IPAC, California Institute of Technology, Pasadena, CA, USA
| | - D L Shupe
- IPAC, California Institute of Technology, Pasadena, CA, USA
| | - I Andreoni
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - Y Sharma
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - R Riddle
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - J van Roestel
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - N Knezevic
- Department of Astronomy, Faculty of Mathematics, University of Belgrade, Belgrade, Serbia
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3
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De K, Kasliwal MM, Ofek EO, Moriya TJ, Burke J, Cao Y, Cenko SB, Doran GB, Duggan GE, Fender RP, Fransson C, Gal-Yam A, Horesh A, Kulkarni SR, Laher RR, Lunnan R, Manulis I, Masci F, Mazzali PA, Nugent PE, Perley DA, Petrushevska T, Piro AL, Rumsey C, Sollerman J, Sullivan M, Taddia F. A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary. Science 2018; 362:201-206. [PMID: 30309948 DOI: 10.1126/science.aas8693] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/31/2017] [Accepted: 07/26/2018] [Indexed: 11/02/2022]
Abstract
Compact neutron star binary systems are produced from binary massive stars through stellar evolution involving up to two supernova explosions. The final stages in the formation of these systems have not been directly observed. We report the discovery of iPTF 14gqr (SN 2014ft), a type Ic supernova with a fast-evolving light curve indicating an extremely low ejecta mass (≈0.2 solar masses) and low kinetic energy (≈2 × 1050 ergs). Early photometry and spectroscopy reveal evidence of shock cooling of an extended helium-rich envelope, likely ejected in an intense pre-explosion mass-loss episode of the progenitor. Taken together, we interpret iPTF 14gqr as evidence for ultra-stripped supernovae that form neutron stars in compact binary systems.
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Affiliation(s)
- K De
- Cahill Centre for Astrophysics, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.
| | - M M Kasliwal
- Cahill Centre for Astrophysics, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - E O Ofek
- Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100, Israel
| | - T J Moriya
- Division of Theoretical Astronomy, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
| | - J Burke
- Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA.,Department of Physics, University of California, Santa Barbara, CA 93106, USA
| | - Y Cao
- Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, USA
| | - S B Cenko
- Astrophysics Science Division, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771, USA.,Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA
| | - G B Doran
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - G E Duggan
- Cahill Centre for Astrophysics, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - R P Fender
- Department of Physics, Astrophysics, University of Oxford, Denys Wilkinson Building, Oxford OX1 3RH, UK
| | - C Fransson
- Oskar Klein Centre, Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
| | - A Gal-Yam
- Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100, Israel
| | - A Horesh
- Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - S R Kulkarni
- Cahill Centre for Astrophysics, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - R R Laher
- Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA
| | - R Lunnan
- Oskar Klein Centre, Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
| | - I Manulis
- Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100, Israel
| | - F Masci
- Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA
| | - P A Mazzali
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool L3 5RF, UK.,Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching bei München, Germany
| | - P E Nugent
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.,Department of Astronomy, University of California, Berkeley, CA, 94720, USA
| | - D A Perley
- Astrophysics Research Institute, Liverpool John Moores University, Liverpool L3 5RF, UK
| | - T Petrushevska
- Oskar Klein Centre, Department of Physics, Stockholm University, 106 91 Stockholm, Sweden.,Centre for Astrophysics and Cosmology, University of Nova Gorica, Vipavska 11c, 5270 Ajdovščina, Slovenia
| | - A L Piro
- The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA
| | - C Rumsey
- Astrophysics Group, Cavendish Laboratory, 19 J J Thomson Avenue, Cambridge CB3 0HE, UK
| | - J Sollerman
- Oskar Klein Centre, Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
| | - M Sullivan
- Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
| | - F Taddia
- Oskar Klein Centre, Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
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4
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Kasliwal MM, Nakar E, Singer LP, Kaplan DL, Cook DO, Van Sistine A, Lau RM, Fremling C, Gottlieb O, Jencson JE, Adams SM, Feindt U, Hotokezaka K, Ghosh S, Perley DA, Yu PC, Piran T, Allison JR, Anupama GC, Balasubramanian A, Bannister KW, Bally J, Barnes J, Barway S, Bellm E, Bhalerao V, Bhattacharya D, Blagorodnova N, Bloom JS, Brady PR, Cannella C, Chatterjee D, Cenko SB, Cobb BE, Copperwheat C, Corsi A, De K, Dobie D, Emery SWK, Evans PA, Fox OD, Frail DA, Frohmaier C, Goobar A, Hallinan G, Harrison F, Helou G, Hinderer T, Ho AYQ, Horesh A, Ip WH, Itoh R, Kasen D, Kim H, Kuin NPM, Kupfer T, Lynch C, Madsen K, Mazzali PA, Miller AA, Mooley K, Murphy T, Ngeow CC, Nichols D, Nissanke S, Nugent P, Ofek EO, Qi H, Quimby RM, Rosswog S, Rusu F, Sadler EM, Schmidt P, Sollerman J, Steele I, Williamson AR, Xu Y, Yan L, Yatsu Y, Zhang C, Zhao W. Illuminating gravitational waves: A concordant picture of photons from a neutron star merger. Science 2017; 358:1559-1565. [PMID: 29038373 DOI: 10.1126/science.aap9455] [Citation(s) in RCA: 441] [Impact Index Per Article: 63.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/14/2017] [Accepted: 10/05/2017] [Indexed: 11/02/2022]
Abstract
Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.
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Affiliation(s)
- M M Kasliwal
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.
| | - E Nakar
- The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel
| | - L P Singer
- Astroparticle Physics Laboratory, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771, USA.,Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA
| | - D L Kaplan
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - D O Cook
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - A Van Sistine
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - R M Lau
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - C Fremling
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - O Gottlieb
- The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel
| | - J E Jencson
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - S M Adams
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - U Feindt
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
| | - K Hotokezaka
- Center for Computational Astrophysics, Simons Foundation, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA.,Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
| | - S Ghosh
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - D A Perley
- Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK
| | - P-C Yu
- Graduate Institute of Astronomy, National Central University, No. 300, Zhongda Road, Zhongli District, Taoyuan City 32001, Taiwan
| | - T Piran
- Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - J R Allison
- Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, New South Wales 2006, Australia.,Australian Research Council Centre of Excellence for All-sky Astrophysics in 3 Dimensions, Australia
| | - G C Anupama
- Indian Institute of Astrophysics, II Block Koramangala, Bangalore 560034, India
| | - A Balasubramanian
- Indian Institute of Science Education and Research, Dr. Homi Bhabha Road, Pashan, Pune 411008, India
| | - K W Bannister
- Australia Telescope National Facility, Astronomy and Space Science, Commonwealth Scientific and Industrial Research Organisation, Post Office Box 76, Epping, New South Wales 1710, Australia
| | - J Bally
- Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 80305, USA
| | - J Barnes
- Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
| | - S Barway
- South African Astronomical Observatory, Post Office Box 9, Observatory, Cape Town 7935, South Africa
| | - E Bellm
- Department of Astronomy, University of Washington, Seattle, WA 98195, USA
| | - V Bhalerao
- Department of Physics, Indian Institute of Technology Bombay, Mumbai 400076, India
| | - D Bhattacharya
- Inter-University Centre for Astronomy and Astrophysics, Post Office Bag 4, Ganeshkhind, Pune 411007, India
| | - N Blagorodnova
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - J S Bloom
- Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA.,Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50B-4206, Berkeley, CA 94720, USA
| | - P R Brady
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - C Cannella
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - D Chatterjee
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - S B Cenko
- Astroparticle Physics Laboratory, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771, USA.,Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA
| | - B E Cobb
- Department of Physics, George Washington University, Washington, DC 20052, USA
| | - C Copperwheat
- Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK
| | - A Corsi
- Department of Physics and Astronomy, Texas Tech University, Box 41051, Lubbock, TX 79409-1051, USA
| | - K De
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - D Dobie
- Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, New South Wales 2006, Australia.,Australian Research Council Centre of Excellence for All-sky Astrophysics, Australia.,Australia Telescope National Facility, Astronomy and Space Science, Commonwealth Scientific and Industrial Research Organisation, Post Office Box 76, Epping, New South Wales 1710, Australia
| | - S W K Emery
- University College London, Mullard Space Science Laboratory, Holmbury St. Mary, Dorking RH5 6NT, UK
| | - P A Evans
- X-ray and Observational Astronomy Research Group, Leicester Institute for Space and Earth Observation, Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK
| | - O D Fox
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
| | - D A Frail
- National Radio Astronomy Observatory, Socorro, NM 87825, USA
| | - C Frohmaier
- Department of Physics and Astronomy, University of Southampton, Southampton, Hampshire SO17 1BJ, UK.,Institute of Cosmology and Gravitation, Dennis Sciama Building, University of Portsmouth, Burnaby Road, Portsmouth PO1 3FX, UK
| | - A Goobar
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
| | - G Hallinan
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - F Harrison
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - G Helou
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
| | - T Hinderer
- Institute of Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - A Y Q Ho
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - A Horesh
- Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - W-H Ip
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
| | - R Itoh
- Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
| | - D Kasen
- Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA.,Department of Physics, University of California, Berkeley, CA 94720, USA
| | - H Kim
- Gemini Observatory, Casilla 603, La Serena, Chile
| | - N P M Kuin
- University College London, Mullard Space Science Laboratory, Holmbury St. Mary, Dorking RH5 6NT, UK
| | - T Kupfer
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - C Lynch
- Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, New South Wales 2006, Australia.,Australian Research Council Centre of Excellence for All-sky Astrophysics, Australia
| | - K Madsen
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - P A Mazzali
- Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK.,Max-Planck Institute for Astrophysics, Garching, Germany
| | - A A Miller
- Center for Interdisciplinary Exploration and Research in Astrophysics and Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208, USA.,The Adler Planetarium, Chicago, IL 60605, USA
| | - K Mooley
- Astrophysics, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
| | - T Murphy
- Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, New South Wales 2006, Australia.,Australian Research Council Centre of Excellence for All-sky Astrophysics, Australia
| | - C-C Ngeow
- Graduate Institute of Astronomy, National Central University, No. 300, Zhongda Road, Zhongli District, Taoyuan City 32001, Taiwan
| | - D Nichols
- Institute of Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - S Nissanke
- Institute of Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - P Nugent
- Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA.,Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50B-4206, Berkeley, CA 94720, USA
| | - E O Ofek
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel
| | - H Qi
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - R M Quimby
- Department of Astronomy, San Diego State University, San Diego, CA 92182, USA.,Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - S Rosswog
- The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
| | - F Rusu
- School of Engineering (EECS), University of California, Merced, CA 95343, USA
| | - E M Sadler
- Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, New South Wales 2006, Australia.,Australian Research Council Centre of Excellence for All-sky Astrophysics, Australia
| | - P Schmidt
- Institute of Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - J Sollerman
- The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
| | - I Steele
- Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK
| | - A R Williamson
- Institute of Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - Y Xu
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA
| | - L Yan
- Division of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.,Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
| | - Y Yatsu
- Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
| | - C Zhang
- Department of Physics, University of Wisconsin, Milwaukee, WI 53201, USA
| | - W Zhao
- School of Engineering (EECS), University of California, Merced, CA 95343, USA
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5
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Goobar A, Amanullah R, Kulkarni SR, Nugent PE, Johansson J, Steidel C, Law D, Mörtsell E, Quimby R, Blagorodnova N, Brandeker A, Cao Y, Cooray A, Ferretti R, Fremling C, Hangard L, Kasliwal M, Kupfer T, Lunnan R, Masci F, Miller AA, Nayyeri H, Neill JD, Ofek EO, Papadogiannakis S, Petrushevska T, Ravi V, Sollerman J, Sullivan M, Taddia F, Walters R, Wilson D, Yan L, Yaron O. iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova. Science 2017; 356:291-295. [PMID: 28428419 DOI: 10.1126/science.aal2729] [Citation(s) in RCA: 139] [Impact Index Per Article: 19.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/25/2016] [Accepted: 03/24/2017] [Indexed: 11/02/2022]
Abstract
We report the discovery of a multiply imaged, gravitationally lensed type Ia supernova, iPTF16geu (SN 2016geu), at redshift z = 0.409. This phenomenon was identified because the light from the stellar explosion was magnified more than 50 times by the curvature of space around matter in an intervening galaxy. We used high-spatial-resolution observations to resolve four images of the lensed supernova, approximately 0.3 arc seconds from the center of the foreground galaxy. The observations probe a physical scale of ~1 kiloparsec, smaller than is typical in other studies of extragalactic gravitational lensing. The large magnification and symmetric image configuration imply close alignment between the lines of sight to the supernova and to the lens. The relative magnifications of the four images provide evidence for substructures in the lensing galaxy.
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Affiliation(s)
- A Goobar
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden.
| | - R Amanullah
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - S R Kulkarni
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - P E Nugent
- Department of Astronomy, University of California, Berkeley, CA 94720, USA.,MS 50B-4206, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
| | - J Johansson
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel
| | - C Steidel
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - D Law
- Space Telescope Science Institute, Baltimore, MD 21218, USA
| | - E Mörtsell
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - R Quimby
- Department of Astronomy, San Diego State University, San Diego, CA 92182, USA.,Kavli IPMU (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Chiba 277-8583, Japan
| | - N Blagorodnova
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - A Brandeker
- Department of Astronomy, Stockholm University, Albanova, SE 10691 Stockholm, Sweden
| | - Y Cao
- eScience Institute and Department of Astronomy, University of Washington, Seattle, WA 98195, USA
| | - A Cooray
- Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA
| | - R Ferretti
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - C Fremling
- Oskar Klein Centre, Department of Astronomy, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - L Hangard
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - M Kasliwal
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - T Kupfer
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - R Lunnan
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA.,Department of Astronomy, Stockholm University, Albanova, SE 10691 Stockholm, Sweden
| | - F Masci
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
| | - A A Miller
- Center for Interdisciplinary Exploration and Research in Astrophysics and Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208, USA.,Adler Planetarium, Chicago, IL 60605, USA
| | - H Nayyeri
- Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA
| | - J D Neill
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - E O Ofek
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel
| | - S Papadogiannakis
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - T Petrushevska
- Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - V Ravi
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - J Sollerman
- Oskar Klein Centre, Department of Astronomy, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - M Sullivan
- Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
| | - F Taddia
- Oskar Klein Centre, Department of Astronomy, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
| | - R Walters
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - D Wilson
- Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA
| | - L Yan
- Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
| | - O Yaron
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel
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6
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Nicholl M, Smartt SJ, Jerkstrand A, Inserra C, McCrum M, Kotak R, Fraser M, Wright D, Chen TW, Smith K, Young DR, Sim SA, Valenti S, Howell DA, Bresolin F, Kudritzki RP, Tonry JL, Huber ME, Rest A, Pastorello A, Tomasella L, Cappellaro E, Benetti S, Mattila S, Kankare E, Kangas T, Leloudas G, Sollerman J, Taddia F, Berger E, Chornock R, Narayan G, Stubbs CW, Foley RJ, Lunnan R, Soderberg A, Sanders N, Milisavljevic D, Margutti R, Kirshner RP, Elias-Rosa N, Morales-Garoffolo A, Taubenberger S, Botticella MT, Gezari S, Urata Y, Rodney S, Riess AG, Scolnic D, Wood-Vasey WM, Burgett WS, Chambers K, Flewelling HA, Magnier EA, Kaiser N, Metcalfe N, Morgan J, Price PA, Sweeney W, Waters C. Slowly fading super-luminous supernovae that are not pair-instability explosions. Nature 2013; 502:346-9. [DOI: 10.1038/nature12569] [Citation(s) in RCA: 204] [Impact Index Per Article: 18.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/10/2013] [Accepted: 08/09/2013] [Indexed: 11/09/2022]
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7
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Watson D, Fynbo JPU, Thöne CC, Sollerman J. No supernovae detected in two long-duration gamma-ray bursts. Philos Trans A Math Phys Eng Sci 2007; 365:1269-75. [PMID: 17296596 DOI: 10.1098/rsta.2006.1994] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/13/2023]
Abstract
There is strong evidence that long-duration gamma-ray bursts (GRBs) are produced during the collapse of a massive star. In the standard version of the collapsar model, a broad-lined and luminous Type Ic core-collapse supernova (SN) accompanies the GRB. This association has been confirmed in observations of several nearby GRBs. Recent observations show that some long-duration GRBs are different. No SN emission accompanied the long-duration GRBs 060505 and 060614 down to limits fainter than any known Type Ic SN and hundreds of times fainter than the archetypal SN 1998bw that accompanied GRB 980425. Multi-band observations of the early afterglows, as well as spectroscopy of the host galaxies, exclude the possibility of significant dust obscuration. Furthermore, the bursts originated in star-forming galaxies, and in the case of GRB 060505, the burst was localized to a compact star-forming knot in a spiral arm of its host galaxy. We find that the properties of the host galaxies, the long duration of the bursts and, in the case of GRB 060505, the location of the burst within its host, all imply a massive stellar origin. The absence of an SN to such deep limits therefore suggests a new phenomenological type of massive stellar death.
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Affiliation(s)
- D Watson
- Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen Ø, Denmark.
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8
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Pian E, Mazzali PA, Masetti N, Ferrero P, Klose S, Palazzi E, Ramirez-Ruiz E, Woosley SE, Kouveliotou C, Deng J, Filippenko AV, Foley RJ, Fynbo JPU, Kann DA, Li W, Hjorth J, Nomoto K, Patat F, Sauer DN, Sollerman J, Vreeswijk PM, Guenther EW, Levan A, O'Brien P, Tanvir NR, Wijers RAMJ, Dumas C, Hainaut O, Wong DS, Baade D, Wang L, Amati L, Cappellaro E, Castro-Tirado AJ, Ellison S, Frontera F, Fruchter AS, Greiner J, Kawabata K, Ledoux C, Maeda K, Møller P, Nicastro L, Rol E, Starling R. An optical supernova associated with the X-ray flash XRF 060218. Nature 2006; 442:1011-3. [PMID: 16943831 DOI: 10.1038/nature05082] [Citation(s) in RCA: 393] [Impact Index Per Article: 21.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/20/2006] [Accepted: 07/10/2006] [Indexed: 11/09/2022]
Abstract
Long-duration gamma-ray bursts (GRBs) are associated with type Ic supernovae that are more luminous than average and that eject material at very high velocities. Less-luminous supernovae were not hitherto known to be associated with GRBs, and therefore GRB-supernovae were thought to be rare events. Whether X-ray flashes--analogues of GRBs, but with lower luminosities and fewer gamma-rays--can also be associated with supernovae, and whether they are intrinsically 'weak' events or typical GRBs viewed off the axis of the burst, is unclear. Here we report the optical discovery and follow-up observations of the type Ic supernova SN 2006aj associated with X-ray flash XRF 060218. Supernova 2006aj is intrinsically less luminous than the GRB-supernovae, but more luminous than many supernovae not accompanied by a GRB. The ejecta velocities derived from our spectra are intermediate between these two groups, which is consistent with the weakness of both the GRB output and the supernova radio flux. Our data, combined with radio and X-ray observations, suggest that XRF 060218 is an intrinsically weak and soft event, rather than a classical GRB observed off-axis. This extends the GRB-supernova connection to X-ray flashes and fainter supernovae, implying a common origin. Events such as XRF 060218 are probably more numerous than GRB-supernovae.
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Affiliation(s)
- E Pian
- Istituto Nazionale di Astrofisica, Trieste Astronomical Observatory, via G. B. Tiepolo 11, I-34131 Trieste, Italy.
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9
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Gehrels N, Sarazin CL, O'Brien PT, Zhang B, Barbier L, Barthelmy SD, Blustin A, Burrows DN, Cannizzo J, Cummings JR, Goad M, Holland ST, Hurkett CP, Kennea JA, Levan A, Markwardt CB, Mason KO, Meszaros P, Page M, Palmer DM, Rol E, Sakamoto T, Willingale R, Angelini L, Beardmore A, Boyd PT, Breeveld A, Campana S, Chester MM, Chincarini G, Cominsky LR, Cusumano G, de Pasquale M, Fenimore EE, Giommi P, Gronwall C, Grupe D, Hill JE, Hinshaw D, Hjorth J, Hullinger D, Hurley KC, Klose S, Kobayashi S, Kouveliotou C, Krimm HA, Mangano V, Marshall FE, McGowan K, Moretti A, Mushotzky RF, Nakazawa K, Norris JP, Nousek JA, Osborne JP, Page K, Parsons AM, Patel S, Perri M, Poole T, Romano P, Roming PWA, Rosen S, Sato G, Schady P, Smale AP, Sollerman J, Starling R, Still M, Suzuki M, Tagliaferri G, Takahashi T, Tashiro M, Tueller J, Wells AA, White NE, Wijers RAMJ. A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225. Nature 2005; 437:851-4. [PMID: 16208363 DOI: 10.1038/nature04142] [Citation(s) in RCA: 471] [Impact Index Per Article: 24.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/31/2005] [Accepted: 08/10/2005] [Indexed: 11/08/2022]
Abstract
Gamma-ray bursts (GRBs) come in two classes: long (> 2 s), soft-spectrum bursts and short, hard events. Most progress has been made on understanding the long GRBs, which are typically observed at high redshift (z approximately 1) and found in subluminous star-forming host galaxies. They are likely to be produced in core-collapse explosions of massive stars. In contrast, no short GRB had been accurately (< 10'') and rapidly (minutes) located. Here we report the detection of the X-ray afterglow from--and the localization of--the short burst GRB 050509B. Its position on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225, which is the location one would expect if the origin of this GRB is through the merger of neutron-star or black-hole binaries. The X-ray afterglow was weak and faded below the detection limit within a few hours; no optical afterglow was detected to stringent limits, explaining the past difficulty in localizing short GRBs.
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Affiliation(s)
- N Gehrels
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
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