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The Prompt X-Ray Emission of Gamma-Ray Burst 980519

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Published 1999 March 22 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation J. J. M. in 't Zand et al 1999 ApJ 516 L57 DOI 10.1086/312002

1538-4357/516/2/L57

Abstract

The prompt X-ray emission from gamma-ray burst (GRB) 980519, as measured with the Wide Field Cameras on board BeppoSAX, is characterized by a strong soft-to-hard-to-soft evolution. An analysis of the evolution of the X-ray spectrum in terms of a single power-law model shows that the photon index evolved from -2.0 to -1.1 to -2.4. The onset of the burst has such a soft spectrum that the 2-27 keV emission appears to precede the ≳107 keV emission of GRB 980519 (as measured with the Burst and Transient Source Experiment) by about 70 s. Nevertheless, we show that this early spectral variation is part of a smooth evolution over the whole burst and that there is no convincing evidence that the early X-rays originate from a physical process that is different from that giving rise to the remainder of the burst.

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10.1086/312002