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Gamma-ray burster counterparts - RadioMany 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.
Document ID
19890050347
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schaefer, Bradley E.
(NASA Goddard Space Flight Center Greenbelt; Maryland, University, College Park, United States)
Cline, Thomas L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Desai, U. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Teegarden, B. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Atteia, J.-L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Barat, C.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Estulin, I. V.
(AN SSSR Institut Kosmicheskikh Issledovanii, Moscow, Ussr)
Evans, W. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Fenimore, E. E.
(Los Alamos National Laboratory NM, United States)
Hurley, K.
(Centre d'Etude Spatiale des Rayonnements, Toulouse, France; California, University Berkeley, United States)
Date Acquired
August 14, 2013
Publication Date
May 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 340
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
89A37718
Distribution Limits
Public
Copyright
Other

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