伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期一, 十二月 15, 2008

Belczynski 2008 高红移暴GRB 080913的观测

主要内容:
目前红移最高: z=6.7.
但前身星依然更可能是PopII而不是PopIII的. (也就是到目前为止还是没有popIII的前身星)

精彩摘抄:


文章信息:

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Title:
On The Origin Of The Highest Redshift Gamma-Ray Burst GRB 080913
Authors:
Belczynski, Krzysztof; Hartmann, Dieter H.; Fryer, Chris L.; Holz, Daniel E.; O'Shea, Brian
Publication:
eprint arXiv:0812.2470
Publication Date:
12/2008
Origin:
ARXIV
Keywords:
Astrophysics
Comment:
13 pages, 5 figures, submitted to ApJ
Bibliographic Code:
2008arXiv0812.2470B

Abstract

GRB 080913, discovered by SWIFT, is the most distant gamma-ray burst (GRB) known to-date, with a spectroscopically determined redshift of z=6.7. The detection of a burst at such an early epoch of the Universe significantly constrains the nature of GRBs and their progenitors. To evaluate these constraints, we perform population synthesis studies of the formation and evolution of early stars and calculate the resulting formation rates of short- and long-duration GRBs at high redshift. The peak of the GRB rate from Population II stars occurs at z=7 for a model with efficient/fast mixing of metals, while it is found at z=3 for an inefficient/slow metallicity evolution model. We show that for at z=6.7 essentially all GRBs originate from Population II stars, independent of the adopted metallicity evolution model. At this epoch Population III (metal free) stars, representing the very first generation of stars, most likely have already completed their evolution, and Population I stars (representing the present population) have just begun forming. We argue that Population II stars (having small, but non-zero metallicity) are the most likely progenitors of both long GRBs (collapsars) and short GRBs (NS-NS or BH-NS mergers) in the redshift range 6\less z \less 10.> Bibtex entry for this abstract Preferred format for this abstract (see Preferences)

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