The redshift of GRB 970508

被引:35
作者
Reichart, DE [1 ]
机构
[1] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
基金
美国国家航空航天局;
关键词
gamma-rays; bursts;
D O I
10.1086/311222
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
GRB 970508 is the second gamma-ray burst (GRB) for which an optical afterglow has been detected. It is the first GRB for which a distance scale has been determined: absorption and emission features in spectra of the optical afterglow place GRB 970508 at a redshift of z greater than or equal to 0.835. The lack of a Ly alpha forest in these spectra further constrains this redshift to be less than z similar to 2.3. I show that the spectrum of the optical afterglow of GRB 970508, once corrected for Galactic absorption, is inconsistent with the relativistic blast-wave model unless a second, redshifted source of extinction is introduced. This second source of extinction may be the yet unobserved host galaxy. I determine its redshift to be z = 1.09(-0.41)(+0.14), which is consistent with the observed redshift of z = 0.835. Redshifts greater than z = 1.40 are ruled out at the 3 sigma confidence level.
引用
收藏
页码:L99 / L101
页数:3
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