Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-11-30
Astronomy and Astrophysics
Astrophysics
4 pages, 2 postscript figures, body of paper abridged in order to fit the four pages of ApJL. Minor corrections. ApJ Letters i
Scientific paper
10.1086/319475
We consider models for the generation of the emission line recently discovered in the X-ray afterglow spectrum of several bursts, and especially of GRB 991216 observed by Chandra. These observations suggest the presence of 0.1-1 solar masses of iron in the vicinity of the bursts. We show that there are strong geometrical and kinematical constraints on the line emitting material. We discuss several classes of models, favoring one where the line photons are produced by reflection off the walls of a wide funnel of semi-opening angle 45 degrees, excavated in a young (a few months old) supernova remnant made of ~10 solar masses with radius 6x10^15 cm, and ~1 solar mass of iron, providing strong support for the SupraNova model.
Fiore Fabrizio
Ghisellini Gabriele
Lazzati Davide
Stella Luigi
Vietri Mario
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