Ulysses/BeppoSAX observations of cosmic gamma-ray-bursts

被引：0
|
作者：
Hurley, K [1 ]
Cline, T
Frontera, F
Dal Fiume, D
Orlandini, M
Costa, E
Piro, L
Feroci, RI
机构：
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Ferrara, I-44100 Ferrara, Italy
[4] CNR, Ist Tesre, I-40129 Bologna, Italy
[5] CNR, Ist Astrofis Spaziale, I-00044 Frascati, Italy
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 69卷 / 1-3期
基金：
美国国家航空航天局;
关键词：
D O I：
10.1016/S0920-5632(98)00317-X
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
BeppoSAX has been added to the 3rd Interplanetary Network of gamma-ray burst detectors. Of the 8 events observed to date by Ulysses and the BeppoSAX Gamma Ray Burst Monitor (GRBM), four have been localized by triangulation, resulting in annuli whose 3 sigma widths are as small as 63''. These data give error boxes whose sizes are sometimes smaller than those obtained with the SAX Wide Field Camera (WFC). They can be used to confirm the association between fading X-ray and optical sources and gamma-ray bursts.
引用
收藏
页码：660 / 663
页数：4
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