The radio counterparts of gamma-ray bursts

Details The radio counterparts of gamma-ray bursts The radio counterparts of gamma-ray bursts

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..563f&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 563-570 (1998).

Computer Science

7

Gamma-Ray Sources, Gamma-Ray Bursts, Radio, Microwave

Scientific paper

In the last three decades sensitive radio searches have been made for prompt emission accompanying a burst, flaring or fading emission on time scales of days to weeks following a burst, and quiescent radio emission from the host object well after the burst has faded from view. These efforts have recently been rewarded with the detection of the radio afterglow from GRB970508. I will summarize all that has been learned from a continuing study of this source at the Very Large Array (VLA). The absence of radio emission from a large number of well-monitored events similar to GRB970508, suggests that detectable radio emission is not a generic consequence of gamma-ray bursts.

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