The 1.4 GH[CLC]z[/CLC] Light Curve of GRB 970508

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 (dNIdγe ∝ γe-p) 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. © 1998. The American Astronomical Society. All rights reserved.