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.

星期二, 十月 30, 2007

Cen 2007 GRB biased trace star formation

主要内容:
GRB history doesn't agree with that of Star formation in well.

精彩摘抄:


文章信息:
Gamma-Ray Bursts May Be Biased Tracers of Star Formation

Authors: Renyue Cen (Princeton), Taotao Fang (UCI)
Abstract: Based on a simulation of galaxy formation in the standard cosmological model, we suggest that a consistent picture for Gamma-Ray Bursts and star formation may be found that is in broad agreement with observations: GRBs preferentially form in low metallicity environments and in galaxies substantially less luminous that L*. We find that the computed formation rate of stars with metallicity less than 0.1Zsun agrees remarkably well with the rate evolution of Gamma-Ray Bursts observed by Swift from z=0 to z=4, whereas the evolution of total star formation rate is weaker by a factor of about 4. Given this finding, we caution that any inference of star formation rate based on observed GRB rate may require a more involved exercise than a simple proportionality.
Comments: submitted to ApJL, 4 pages
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0710.4370v1 [astro-ph]

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