Integral monitoring of the bright neutron star low mass X-ray binaries: Preliminary results on GX 17+2

被引：0

作者：

Piraino, S ^{[1
]}

Santangelo, A ^{[1
]}

Ferrigno, C ^{[1
]}

Segreto, A ^{[1
]}

La Barbera, A ^{[1
]}

Bazzano, A ^{[1
]}

Del Santo, M ^{[1
]}

Natalucci, L ^{[1
]}

Ubertini, P ^{[1
]}

Paizis, A ^{[1
]}

Courvoisier, TJL ^{[1
]}

Chernyakova, M ^{[1
]}

Walter, R ^{[1
]}

Vilhu, O ^{[1
]}

Farinelli, R ^{[1
]}

Frontera, F ^{[1
]}

Lund, N ^{[1
]}

Beckmann, V ^{[1
]}

机构：

[1] CNR, IASF, Sez Palermo, I-90146 Palermo, Italy

来源：

PROCEEDINGS OF THE 5TH INTEGRAL WORKSHOP ON THE INTEGRAL UNIVERSE | 2004年 / 552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：

GX17+2 is a bright Neutron Star Low Mass X-ray Binary. Albeit significant results were obtained from previous campaigns, many open points still remain in the understanding of such a source, in particular the origin (thermal or not) of the hard component and its behavior with the spectral state. INTEGRAL offers the opportunity to reduce these ambiguities. Combining data from JEM-X, IBIS and SPI to provide a complete soft to hard energy coverage, we report preliminary results based on the first year Core Program observations of GX 17+2.

引用

页码：369 / 372

页数：4

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