NEUTRON-STARS AND THE DISTANCE TO GAMMA-RAY BURSTERS

被引：1

作者：

DERMER, CD ^{[1
]}

HURLEY, KC ^{[1
]}

机构：

[1] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1991年 / 103卷 / 666期

关键词：

GAMMA-RAY BURST SOURCES; NEUTRON STARS;

D O I：

10.1086/132879

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Assuming that gamma-ray bursts originate from galactic neutron stars, we outline an analytic method for studying their statistical properties. If a significant fraction of all neutron stars are born with space velocities less-than-or-similar-to km s-1, as suggested by studies of pulsar statistics, then the sampling distance to gamma-ray burst sources should be less than approximately several hundred pc. These results have important implications on theories of radio pulsar evolution and magnetic-field decay.

引用

页码：774 / 776

页数：3

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