IBIS detectability of the Hard X-ray tailed sample of bursters

被引：0

作者：

Bazzano, A ^{[1
]}

De Cesare, G ^{[1
]}

Cocchi, M ^{[1
]}

Natalucci, L ^{[1
]}

Ubertini, P ^{[1
]}

机构：

[1] CNR, Ist Astrofis Spaziale, I-00133 Rome, Italy

来源：

FIFTH COMPTON SYMPOSIUM | 2000年 / 510卷

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：

During the 2.5 years of Galactic Bulge Monitoring with the WFC on board the Beppo-SAX satellite new X-Ray Burst sources have been discovered. Some of these sources have also been promptly observed on a wide energy band by using the Narrow Field instruments of the Satellite and a high energy component up to 200 keV has been detected. Moreover bursts behaviour has been discovered with the WFC for 4 more sources previously observed with other high energy instruments enlarging the sample of studied objects. These results support the existence of such a class of previously suggested hard X-ray emitters that are very promising for the future IBIS/INTEGRAL CORE programme observations (Galactic Plane Survey and the Galactic Centre Deep Exposure). Simulation results on the IBIS view on this class of object will be presented.

引用

页码：698 / 702

页数：5

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