The Discovery of the Radio Afterglow From the Optically Dim Gamma-Ray Burst of March 29, 1998

Details The Discovery of the Radio Afterglow From the Optically Dim Gamma-Ray Burst of March 29, 1998 The Discovery of the Radio Afterglow From the Optically Dim Gamma-Ray Burst of March 29, 1998

1998-05-27

arxiv.org/abs/astro-ph/9805333v1

Astronomy and Astrophysics

Astrophysics

in press at ApJ Letters, 12 page LaTeX document includes 2 postscript figures

Scientific paper

10.1086/311513

We report on the discovery of a variable radio source, VLA J070238.0+385044, associated with the proposed x-ray counterpart, 1SAX J0702.6+3850 of GRB 980329. The source was monitored from one day after the burst to one month later at centimeter wavelengths (1.4, 4.9, 8.3 and 15 GHz; Very Large Array -- VLA), and in the 3-mm band (90 GHz; Owen Valley Radio Observatory -- OVRO). Based on its variability, compactness and spectrum, we identify VLA J070238.0+385044 as the afterglow from GRB 980329. We interpret the rapid flux density variations as interstellar scintillation and the sharp turnover in the radio spectrum below 13 GHz as arising from synchrotron self-absorption. This suggests that the angular diameter of the fireball from GRB 980329 was of order a few microarcseconds in the first two weeks. The absence of a readily detectable afterglow in the optical, but clear detections in both the radio and infrared, can be understood as the result of extinction by dust. In this context it is interesting to note that half of all well-localized gamma-ray bursts have no optical counterpart. Based on our study of GRB 980329 we suggest that the progenitors of a sizable fraction of gamma-ray bursts are associated with regions of moderate to high gas density.

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