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Hurley-Walker N, Rea N, McSweeney SJ, Meyers BW, Lenc E, Heywood I, Hyman SD, Men YP, Clarke TE, Coti Zelati F, Price DC, Horváth C, Galvin TJ, Anderson GE, Bahramian A, Barr ED, Bhat NDR, Caleb M, Dall'Ora M, de Martino D, Giacintucci S, Morgan JS, Rajwade KM, Stappers B, Williams A. A long-period radio transient active for three decades. Nature 2023; 619:487-490. [PMID: 37468588 DOI: 10.1038/s41586-023-06202-5] [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: 02/07/2023] [Accepted: 05/11/2023] [Indexed: 07/21/2023]
Abstract
Several long-period radio transients have recently been discovered, with strongly polarized coherent radio pulses appearing on timescales between tens to thousands of seconds1,2. In some cases, the radio pulses have been interpreted as coming from rotating neutron stars with extremely strong magnetic fields, known as magnetars; the origin of other, occasionally periodic and less-well-sampled radio transients is still debated3. Coherent periodic radio emission is usually explained by rotating dipolar magnetic fields and pair-production mechanisms, but such models do not easily predict radio emission from such slowly rotating neutron stars and maintain it for extended times. On the other hand, highly magnetic isolated white dwarfs would be expected to have long spin periodicities, but periodic coherent radio emission has not yet been directly detected from these sources. Here we report observations of a long-period (21 min) radio transient, which we have labelled GPM J1839-10. The pulses vary in brightness by two orders of magnitude, last between 30 and 300 s and have quasiperiodic substructure. The observations prompted a search of radio archives and we found that the source has been repeating since at least 1988. The archival data enabled constraint of the period derivative to <3.6 × 10-13 s s-1, which is at the very limit of any classical theoretical model that predicts dipolar radio emission from an isolated neutron star.
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Affiliation(s)
- N Hurley-Walker
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia.
| | - N Rea
- Institute of Space Sciences (ICE), Consejo Superior de Investigaciones Científicas (CSIC), Barcelona, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
| | - S J McSweeney
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - B W Meyers
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - E Lenc
- Australia Telescope National Facility (ATNF), CSIRO Space & Astronomy, Epping, New South Wales, Australia
| | - I Heywood
- Astrophysics, University of Oxford, Oxford, UK
- Department of Physics & Electronics, Rhodes University, Makhanda, South Africa
- South African Radio Astronomy Observatory (SARAO), Cape Town, South Africa
| | - S D Hyman
- Department of Engineering and Physics, Sweet Briar College, Sweet Briar, VA, USA
| | - Y P Men
- Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - T E Clarke
- Remote Sensing Division, U.S. Naval Research Laboratory, Washington, DC, USA
| | - F Coti Zelati
- Institute of Space Sciences (ICE), Consejo Superior de Investigaciones Científicas (CSIC), Barcelona, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
| | - D C Price
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - C Horváth
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - T J Galvin
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
- CSIRO, Space and Astronomy, Bentley, Western Australia, Australia
| | - G E Anderson
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - A Bahramian
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - E D Barr
- Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - N D R Bhat
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - M Caleb
- Sydney Institute for Astronomy, School of Physics, The University of Sydney, Sydney, New South Wales, Australia
- ASTRO3D: ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions, Canberra, Australian Capital Territory, Australia
| | - M Dall'Ora
- INAF Capodimonte Astronomical Observatory Naples, Naples, Italy
| | - D de Martino
- INAF Capodimonte Astronomical Observatory Naples, Naples, Italy
| | - S Giacintucci
- Remote Sensing Division, U.S. Naval Research Laboratory, Washington, DC, USA
| | - J S Morgan
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
| | - K M Rajwade
- ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, The Netherlands
| | - B Stappers
- Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Manchester, UK
| | - A Williams
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia, Australia
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Hurley-Walker N, Zhang X, Bahramian A, McSweeney SJ, O'Doherty TN, Hancock PJ, Morgan JS, Anderson GE, Heald GH, Galvin TJ. A radio transient with unusually slow periodic emission. Nature 2022; 601:526-530. [PMID: 35082416 DOI: 10.1038/s41586-021-04272-x] [Citation(s) in RCA: 12] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/30/2021] [Accepted: 11/19/2021] [Indexed: 11/09/2022]
Abstract
The high-frequency radio sky is bursting with synchrotron transients from massive stellar explosions and accretion events, but the low-frequency radio sky has, so far, been quiet beyond the Galactic pulsar population and the long-term scintillation of active galactic nuclei. The low-frequency band, however, is sensitive to exotic coherent and polarized radio-emission processes, such as electron-cyclotron maser emission from flaring M dwarfs1, stellar magnetospheric plasma interactions with exoplanets2 and a population of steep-spectrum pulsars3, making Galactic-plane searches a prospect for blind-transient discovery. Here we report an analysis of archival low-frequency radio data that reveals a periodic, low-frequency radio transient. We find that the source pulses every 18.18 min, an unusual periodicity that has, to our knowledge, not been observed previously. The emission is highly linearly polarized, bright, persists for 30-60 s on each occurrence and is visible across a broad frequency range. At times, the pulses comprise short-duration (<0.5 s) bursts; at others, a smoother profile is observed. These profiles evolve on timescales of hours. By measuring the dispersion of the radio pulses with respect to frequency, we have localized the source to within our own Galaxy and suggest that it could be an ultra-long-period magnetar.
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Affiliation(s)
- N Hurley-Walker
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia.
| | - X Zhang
- CSIRO, Space and Astronomy, Bentley, Western Australia, Australia.,Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, China
| | - A Bahramian
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - S J McSweeney
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - T N O'Doherty
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - P J Hancock
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - J S Morgan
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - G E Anderson
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
| | - G H Heald
- CSIRO, Space and Astronomy, Bentley, Western Australia, Australia
| | - T J Galvin
- International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia
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Veres P, Bhat PN, Briggs MS, Cleveland WH, Hamburg R, Hui CM, Mailyan B, Preece RD, Roberts OJ, von Kienlin A, Wilson-Hodge CA, Kocevski D, Arimoto M, Tak D, Asano K, Axelsson M, Barbiellini G, Bissaldi E, Dirirsa FF, Gill R, Granot J, McEnery J, Omodei N, Razzaque S, Piron F, Racusin JL, Thompson DJ, Campana S, Bernardini MG, Kuin NPM, Siegel MH, Cenko SB, O’Brien P, Capalbi M, Daì A, De Pasquale M, Gropp J, Klingler N, Osborne JP, Perri M, Starling RLC, Tagliaferri G, Tohuvavohu A, Ursi A, Tavani M, Cardillo M, Casentini C, Piano G, Evangelista Y, Verrecchia F, Pittori C, Lucarelli F, Bulgarelli A, Parmiggiani N, Anderson GE, Anderson JP, Bernardi G, Bolmer J, Caballero-García MD, Carrasco IM, Castellón A, Segura NC, Castro-Tirado AJ, Cherukuri SV, Cockeram AM, D’Avanzo P, Di Dato A, Diretse R, Fender RP, Fernández-García E, Fynbo JPU, Fruchter AS, Greiner J, Gromadzki M, Heintz KE, Heywood I, van der Horst AJ, Hu YD, Inserra C, Izzo L, Jaiswal V, Jakobsson P, Japelj J, Kankare E, Kann DA, Kouveliotou C, Klose S, Levan AJ, Li XY, Lotti S, Maguire K, Malesani DB, Manulis I, Marongiu M, Martin S, Melandri A, Michałowski MJ, Miller-Jones JCA, Misra K, Moin A, Mooley KP, Nasri S, Nicholl M, Noschese A, Novara G, Pandey SB, Peretti E, del Pulgar CJP, Pérez-Torres MA, Perley DA, Piro L, Ragosta F, Resmi L, Ricci R, Rossi A, Sánchez-Ramírez R, Selsing J, Schulze S, Smartt SJ, Smith IA, Sokolov VV, Stevens J, Tanvir NR, Thöne CC, Tiengo A, Tremou E, Troja E, de Ugarte Postigo A, Valeev AF, Vergani SD, Wieringa M, Woudt PA, Xu D, Yaron O, Young DR. Observation of inverse Compton emission from a long γ-ray burst. Nature 2019; 575:459-463. [DOI: 10.1038/s41586-019-1754-6] [Citation(s) in RCA: 92] [Impact Index Per Article: 18.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/20/2019] [Accepted: 10/18/2019] [Indexed: 11/09/2022]
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van Velzen S, Anderson GE, Stone NC, Fraser M, Wevers T, Metzger BD, Jonker PG, van der Horst AJ, Staley TD, Mendez AJ, Miller-Jones JCA, Hodgkin ST, Campbell HC, Fender RP. A radio jet from the optical and x-ray bright stellar tidal disruption flare ASASSN-14li. Science 2016; 351:62-5. [PMID: 26612833 DOI: 10.1126/science.aad1182] [Citation(s) in RCA: 120] [Impact Index Per Article: 15.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/31/2015] [Accepted: 11/13/2015] [Indexed: 11/02/2022]
Affiliation(s)
- S. van Velzen
- Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA
| | - G. E. Anderson
- Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
- International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth WA 6845, Australia
| | - N. C. Stone
- Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
| | - M. Fraser
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
| | - T. Wevers
- Department of Astrophysics, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
| | - B. D. Metzger
- Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
| | - P. G. Jonker
- Department of Astrophysics, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, Netherlands
- SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands
| | - A. J. van der Horst
- Department of Physics, The George Washington University, 725 21st Street NW, Washington, DC 20052, USA
| | - T. D. Staley
- Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
| | - A. J. Mendez
- Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA
| | - J. C. A. Miller-Jones
- International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth WA 6845, Australia
| | - S. T. Hodgkin
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
| | - H. C. Campbell
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
| | - R. P. Fender
- Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
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Hurley-Walker N, Galvin TJ, Duchesne SW, Zhang X, Morgan J, Hancock PJ, An T, Franzen TMO, Heald G, Ross K, Vernstrom T, Anderson GE, Gaensler BM, Johnston-Hollitt M, Kaplan DL, Riseley CJ, Tingay SJ, Walker M. GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended (GLEAM-X) I: Survey Description and Initial Data Release. Publ Astron Soc Aust 2015; 32:e025. [PMID: 35494410 PMCID: PMC7612673 DOI: 10.1017/pasa.2015.26] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
We describe a new low-frequency wideband radio survey of the southern sky. Observations covering 72-231MHz and Declinations south of +30° have been performed with the Murchison Widefield Array "extended" Phase I I configuration over 2018-2020 and will be processed to form data products including continuum and polarisation images and mosaics, multi-frequency catalogues, transient search data, and ionospheric measurements. From a pilot field described in this work, we publish an initial data release covering 1,447 deg2 over 4 h≤ RA≤ 13 h, -32.7° ≤ Dec ≤ -20.7°. We process twenty frequency bands sampling 72-231 MHz, with a resolution of 2'-45″, and produce a wideband source-finding image across 170-231MHz with a root-mean-square noise of 1.27 ± 0.15 mJy beam-1. Source-finding yields 79,124 components, of which 71,320 are fitted spectrally. The catalogue has a completeness of 98% at ~ 50 mJy, and a reliability of 98.2% at 5σ rising to 99.7% at 7σ. A catalogue is available from Vizier; images are made available on the GLEAM-X VO server and SkyView. This is the first in a series of data releases from the GLEAM-X survey.
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Affiliation(s)
- N Hurley-Walker
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
| | - T J Galvin
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
| | - S W Duchesne
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
| | - X Zhang
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
- Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Rd, Shanghai, 200030, China
| | - J Morgan
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
| | - P J Hancock
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
- Curtin Institute for Computation, Curtin University, GPO Box U1987, Perth WA 6845
| | - T An
- Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Rd, Shanghai, 200030, China
| | - T M O Franzen
- ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, The Netherlands
| | - G Heald
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
| | - K Ross
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
| | - T Vernstrom
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
- International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Hwy, 6009 Crawley, Australia
| | - G E Anderson
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
| | - B M Gaensler
- Dunlap Institute for Astronomy and Astrophysics, 50 St. George St, University of Toronto, ON M5S 3H4, Canada
| | - M Johnston-Hollitt
- Curtin Institute for Computation, Curtin University, GPO Box U1987, Perth WA 6845
| | - D L Kaplan
- Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, WI 53201, USA
| | - C J Riseley
- CSIRO Space & Astronomy, PO Box 1130, Bentley WA 6102, Australia
- Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, via P. Gobetti 93/2, 40129 Bologna, Italy
- INAF - Istituto di Radioastronomia, via P. Gobetti 101, 40129 Bologna, Italy
| | - S J Tingay
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
| | - M Walker
- International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia
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Cohen Y, Anderson GE, Chinkin LR, Pascoe G, Schmidt CE, Winer A. The Valdez Air Health Study. RCAC Valdez Air Study Review Committee. Risk Anal 1994; 14:887-893. [PMID: 7846322 DOI: 10.1111/j.1539-6924.1994.tb00051.x] [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: 05/22/2023]
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Affiliation(s)
- R D Marciani
- Department of Veterans Affairs, University of Kentucky College of Dentistry, Lexington
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Abstract
Microscopic images of a test chart hidden behind a slab of a highly scattering medium were significantly improved by incorporation of a spatial filter located at the back Fourier-transform plane of the objective lens of a microscope. The image quality was shown to be improved further by detection of only the early-arriving photons through time-resolved detection in combination with spatial filtering.
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Bolen GZ, Anderson GE, Huddleson JR, Riley JB, Sutton RG, Bishop DG. Clinical accuracy of continuous hemoglobin oxygen saturation monitoring devices. J Extra Corpor Technol 1989; 22:61-6. [PMID: 10171101] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 02/11/2023]
Abstract
Three devices used to measure hemoglobin oxygen saturation in the extracorporeal circuit were studied and compared to a control. The Baxter Bentley OxySat, Oximetrix Accusat, and Radiometer ABL4 blood gas monitor were compared to a control, the IL 282 Co-Oximeter. Fifty-one sample points were obtained during all phases of cardiopulmonary bypass with results as follows: table: see text. The Accusat was found to be a statistically more accurate means of monitoring hemoglobin oxygen saturations during cardiopulmonary bypass than the ABL4 and the OxySat. All devices had significant correlation with the control and with each other.
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Affiliation(s)
- G Z Bolen
- Department of Extracorporeal Circulation Technology, Medical University of South Carolina, Charleston 29425
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Sutherland DE, Najarian JS, Greenberg BZ, Senske BJ, Anderson GE, Francis RS, Goetz FC. Hormonal and metabolic effects of a pancreatic endocrine graft. Vascularized segmental transplantation in insulin-dependent diabetic patients. Ann Intern Med 1981; 95:537-41. [PMID: 6794405 DOI: 10.7326/0003-4819-95-5-537] [Citation(s) in RCA: 60] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 01/21/2023] Open
Abstract
A new modification of pancreas transplant technique, the vascularized segmental intraperitoneal graft without duct ligation, has provided reversal of insulin-dependent (type I) diabetes mellitus for as long as 2 years of comfortable life. Although the risks associated with immunosuppression remain high (two of the 12 patients have died of early postoperative infection), selected data are presented from six cases to show the following striking hormonal and metabolic results after transplantation and withdrawal of insulin: restoration of normal beta cell function as shown by 24-hour urine C-peptide excretion and acutely responsive serum insulin, restoration of normal suppressibility of plasma glucagon, elimination of ketosis and negative nitrogen balance, normal fasting plasma glucose and glycosylated hemoglobin, and normal or near-normal glucose tolerance. These results provide a standard for current explorations of new ways of treating insulin-dependent diabetes.
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11
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Reiter LW, Anderson GE, Laskey JW, Cahill DF. Developmental and behavioral changes in the rat during chronic exposure to lead. Environ Health Perspect 1975; 12:119-23. [PMID: 1227852 PMCID: PMC1475028 DOI: 10.1289/ehp.7512119] [Citation(s) in RCA: 87] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/18/2023]
Abstract
Young male and female Sprague-Dawley rats were given drinking water containing 5 or 50 ppm Pb for 40 days prior to mating. Pregnant females were continued on these regimens throughout gestation and lactation. After weaning the offspring were similarly exposed through adulthood. Reflex development, body weights, and locomotor activity were measured in the offspring. Significant delays were noted in the development of the righting reflex at 5 and 50 ppm and in eye opening at 50 ppm. No difference was observed in development of the startle reflex at either dose. Mean body weights of treatment groups during this developmental period were not significantly different from controls. Locomotor activity was measured in adult males utilizing a residential maze. Both levels of lead produced a significant reduction in locomotor activity. When groups were treated with d-amphetamine (4.0 mg/kg subcutaneous), lead treatment caused a dose-related diminution in the amphetamine-induced hyperactivity. These results indicate that rats exposed to low levels of lead from conception until adulthood show a delay in nervous system development. As adults, these animals exhibit hypoactivity and decreased responsiveness to amphetamine.
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12
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14
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Lappenbusch WL, Gillespie LJ, Leach WM, Anderson GE. Effect of 2450-MHz microwaves on the radiation response of x-irradiated Chinese hamsters. Radiat Res 1973; 54:294-303. [PMID: 4703889] [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: 01/11/2023]
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15
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Mati JK, Anderson GE, Carty MJ, McGlashan HE. A second look into the problem of primary infertility in Kenya. East Afr Med J 1973; 50:94-7. [PMID: 4723299] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Key Words] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/12/2023]
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16
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Meng HC, Anderson GE. The use of xylitol in long-term parenteral nutrition in dogs. Z Ernahrungswiss Suppl 1973; 15:54-68. [PMID: 4201154 DOI: 10.1007/978-3-662-41451-4_6] [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: 01/09/2023]
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17
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Stirrat GM, Anderson GE, Grant O. The effectiveness of stilboestrol in the suppression on postpartum lactation. J Obstet Gynaecol Br Commonw 1968; 75:313-5. [PMID: 4868189 DOI: 10.1111/j.1471-0528.1968.tb02084.x] [Citation(s) in RCA: 17] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 01/12/2023]
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