Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-03-20
Astrophys.J. 558 (2001) 442-447
Astronomy and Astrophysics
Astrophysics
19 pages, 3 fig.s, minor revisions, accepted for publication in ApJ
Scientific paper
10.1086/322467
We present X-ray observations of the afterglow of GRB000926 performed around and after the break observed in the optical light curve two days after the burst. The steep X-ray light curve observed around the break confirms the presence of this feature in X-rays. However, the spectral and temporal properties are not consistent with a standard jet scenario based on synchrotron emission, requiring a more complicated model. We find that X-ray and optical data are compatible with a moderately collimated fireball (with opening angle $\theta\approx25 \deg$) expanding in a dense medium ($n\approx 4\times 10^4$ cm$^{-3}$). This produces two breaks in the light curve. The first, at $t\approx$ 2 days, is due to jet behavior. The second, around 5 days, is attributed to the transition of the fireball to a non-relativistic expansion. This transition predicts a{\it flattening} of the light curve, that explains the late X-ray measurement in excess above the extrapolation of the simple jet scenario, and is also consistent with optical data.
Antonelli Lucio Angelo
Costa Edgar
Feroci Marco
Frail Dale A.
Garcia Murillo R.
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