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：
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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.
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页码：698 / 702
页数：5
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