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The 1.4 GHz Light Curve of GRB 970508

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Published 1998 June 8 © 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation T. J. Galama et al 1998 ApJ 500 L101 DOI 10.1086/311424

1538-4357/500/2/L101

Abstract

We report on Westerbork 1.4 GHz radio observations of the radio counterpart to γ-ray burst GRB 970508, between 0.80 and 138 days after this event. The 1.4 GHz light curve shows a transition from optically thick to thin emission between 39 and 54 days after the event. We derive the slope p of the spectrum of injected electrons (dN/dγe∝γ−pe) in two independent ways, which yield values very close to p=2.2. This is in agreement with a relativistic dynamically near-adiabatic blast-wave model whose emission is dominated by synchrotron radiation and in which a significant fraction of the electrons cool fast.

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10.1086/311424