Gamma-ray burster counterparts - Radio

Details Gamma-ray burster counterparts - Radio Gamma-ray burster counterparts - Radio

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..455s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 455-457.

Astronomy and Astrophysics

Astronomy

28

Gamma Ray Bursts, Neutron Stars, Radio Sources (Astronomy), Very Large Array (Vla), Circular Polarization, Linear Polarization, Stellar Rotation

Scientific paper

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.

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