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A&A 389, L74-L77 (2002)
DOI: 10.1051/0004-6361:20020852
Letter
X-ray spectral diagnostics of the immediate environment of GRB 991216
D. R. Ballantyne1, E. Ramirez-Ruiz1, D. Lazzati1 and L. Piro21 Institute of Astronomy, University of Cambridge, Madingley Road, CB3 0HA Cambridge, UK
e-mail: drb,enrico,lazzati@ast.cam.ac.uk
2 Istituto di Astrofisica Spaziale, CNR, Via del Fosso del Cavaliere 100, 00133 Roma, Italy
e-mail: piro@ias.rm.cnr.it
(Received 15 April 2002 / Accepted 6 June 2002)
Abstract
The recent report of iron line features in the afterglow of
the gamma-ray burst (GRB) 991216 has important implications for the
properties of the radiating material and hence the nature of the
immediate burst environment. We argue that the putative strong Fe
emission line can be attributed to the reflected emission from
Thomson-thick matter which is illuminated by a power-law
continuum. The ionization parameter of the material (i.e., the flux to
density ratio) is around
103, resulting in a Fe K
line from
He-like iron. A supersolar abundance of iron is not required by the
data. Interestingly, the ionizing continuum must be harder than the
observed one. We interpret this as due to the fact that the
observed continuum is dominated by the standard blast wave emission,
while the line is produced by reprocessing material located at much
smaller radii.
Key words: gamma rays: bursts -- X-rays: general -- radiation mechanisms: non-thermal -- line: formation
Offprint request: D. Ballantyne, drb@ast.cam.ac.uk
SIMBAD Objects
© ESO 2002
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