期刊
ASTROPHYSICAL JOURNAL
卷 605, 期 2, 页码 819-822出版社
IOP PUBLISHING LTD
DOI: 10.1086/382503
关键词
early universe; gamma rays : bursts; stars : formation
It is known that some observed gamma-ray bursts (GRBs) are produced at cosmological distances and that the GRB production rate may follow the star formation rate. We model the BATSE-detected intensity distribution of long GRBs in order to determine their space density distribution and opening angle distribution. Our main results are: the lower and upper distance limits to the GRB production are z approximate to 0.24 and > 10, respectively; the GRB opening angle follows an exponential distribution and the mean opening angle is about 0.03 radians; and the peak luminosity appears to be a better standard candle than the total energy of a GRB.
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