Ulysses/BeppoSAX observations of cosmic gamma-ray bursts

被引：0

作者：

Hurley, K ^{[1
]}

Cline, T ^{[1
]}

Frontera, F ^{[1
]}

Dal Fiume, D ^{[1
]}

Orlandini, M ^{[1
]}

Costa, E ^{[1
]}

Piro, L ^{[1
]}

Feroci, M ^{[1
]}

机构：

[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

来源：

ACTIVE X-RAY SKY: RESULTS FROM BEPPOSAX AND RXTE | 1998年

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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. (WPC). They san be used to confirm the association between fading X-ray and optical sources and gamma-ray bursts.

引用

页码：660 / 663

页数：4

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