Gamma-ray burster counterparts - Radio
Many observers and theorists have suggested that gamma-ray bursters (GRBs) are related to highly magnetized rotating, neutron stars, in which case an analogy with pulsars implies that GRBs would be prodigious emitters of polarized radio emission during quiescence. The paper reports on a survey condu...
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| Veröffentlicht in: | Astrophys. J.; (United States) 1989-05, Vol.340 (1), p.455-457 |
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| container_title | Astrophys. J.; (United States) |
| container_volume | 340 |
| creator | Schaefer, Bradley E. Cline, Thomas L. Desai, U. D. Teegarden, B. J. Atteia, J.-L. Barat, C. Estulin, I. V. Evans, W. D. Fenimore, E. E. Hurley, K. |
| description | Many observers and theorists have suggested that gamma-ray bursters (GRBs) are related to highly magnetized rotating, neutron stars, in which case an analogy with pulsars implies that GRBs would be prodigious emitters of polarized radio emission during quiescence. The paper reports on a survey conducted with the Very Large Array radio telescope of 10 small GRB error regions for quiescent radio emission at wavelengths of 2, 6, and 20 cm. The sensitivity of the survey varied from 0.1 to 0.8 mJy. The observations did indeed reveal four radio sources inside the GRB error regions. |
| doi_str_mv | 10.1086/167407 |
| format | Article |
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E.</creatorcontrib><creatorcontrib>Hurley, K.</creatorcontrib><creatorcontrib>Maryland Univ., College Park (USA)</creatorcontrib><creatorcontrib>Institut Kosmicheskikh Issledovanii, Moscow (USSR)</creatorcontrib><creatorcontrib>NASA, Goddard Space Flight Center, Greenbelt, MD (USA)</creatorcontrib><creatorcontrib>Los Alamos National Lab., NM (USA)</creatorcontrib><creatorcontrib>Centre d'Etude Spatiale des Rayonnements, Toulouse (France)</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Schaefer, Bradley E.</au><au>Cline, Thomas L.</au><au>Desai, U. D.</au><au>Teegarden, B. J.</au><au>Atteia, J.-L.</au><au>Barat, C.</au><au>Estulin, I. V.</au><au>Evans, W. D.</au><au>Fenimore, E. E.</au><au>Hurley, K.</au><aucorp>Maryland Univ., College Park (USA)</aucorp><aucorp>Institut Kosmicheskikh Issledovanii, Moscow (USSR)</aucorp><aucorp>NASA, Goddard Space Flight Center, Greenbelt, MD (USA)</aucorp><aucorp>Los Alamos National Lab., NM (USA)</aucorp><aucorp>Centre d'Etude Spatiale des Rayonnements, Toulouse (France)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gamma-ray burster counterparts - Radio</atitle><jtitle>Astrophys. J.; (United States)</jtitle><date>1989-05-01</date><risdate>1989</risdate><volume>340</volume><issue>1</issue><spage>455</spage><epage>457</epage><pages>455-457</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>Many observers and theorists have suggested that gamma-ray bursters (GRBs) are related to highly magnetized rotating, neutron stars, in which case an analogy with pulsars implies that GRBs would be prodigious emitters of polarized radio emission during quiescence. The paper reports on a survey conducted with the Very Large Array radio telescope of 10 small GRB error regions for quiescent radio emission at wavelengths of 2, 6, and 20 cm. The sensitivity of the survey varied from 0.1 to 0.8 mJy. The observations did indeed reveal four radio sources inside the GRB error regions.</abstract><cop>Legacy CDMS</cop><pub>University of Chicago Press</pub><doi>10.1086/167407</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | Astrophys. J.; (United States), 1989-05, Vol.340 (1), p.455-457 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_167407 |
| source | NASA Technical Reports Server; Alma/SFX Local Collection |
| subjects | 640101 - Astrophysics & Cosmology- Cosmic Radiation 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources Astronomy Astrophysics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC GAMMA BURSTS COSMIC RADIATION COSMIC RADIO SOURCES Earth, ocean, space ELECTROMAGNETIC RADIATION ERRORS Exact sciences and technology GAMMA RADIATION Gamma-ray sources gamma-ray bursts IONIZING RADIATIONS MOTION NEUTRON STARS ORIGIN POLARIZATION PRIMARY COSMIC RADIATION PULSARS RADIATIONS ROTATION STARS Stellar systems. Galactic and extragalactic objects and systems. The universe TELESCOPES Unidentified sources and radiation outside the solar system |
| title | Gamma-ray burster counterparts - Radio |
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