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A&A 407, 393-402 (2003)
DOI: 10.1051/0004-6361:20030871
Emission and absorption lines of gamma-ray bursts affected by the relativistic motion of fireball ejecta
Yi-Ping QinNational Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming, Yunnan 650011, PR China
(Received 29 November 2002 / Accepted 12 May 2003)
Abstract
We display by numerical calculation how rest frame spectral lines
appear in the observed spectrum of gamma-ray bursts due to the
Doppler effect in the fireball framework. The analysis shows that:
a) in the spectrum of a relativistically expanding fireball, all
rest frame lines would shift to higher energy bands and would be
significantly smoothed; b) rest frame weak narrow emission lines
as well as narrow absorption lines and absorption line forests
would be smoothed and would hardly be detectable; c) the features
of rest frame broad emission lines as well as both strong and weak
broad absorption lines would remain almost unchanged and therefore
would be easier to detect; d) deep gaps caused by rest frame broad
absorption lines would be significantly filled; e) a rest frame
emission line forest would form a single broad line feature; f)
the observed relative width of the rest frame very narrow line
would approach
0.162; g) when the Lorentz factor
is
large enough, the observed line frequency
and the
rest frame line frequency
would be related by
. We also investigate
the effect of time dependence of the line intensity and the effect
of variation of
. We find that the feature of rest frame
dimming narrow emission lines would disappear when
is
very large. The form of emission lines would be sharp on both
edges when
varies with time. This phenomenon depends not
only on the initial Lorentz factor but also on the observation
time.
Key words: gamma-rays: bursts -- gamma-rays: theory -- radiation mechanisms: nonthermal -- relativity
© ESO 2003
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