Spectral/timing evolution of black-hole binaries

被引：5

作者：

Belloni, Tomaso M. ^{[1
]}

机构：

[1] INAF Osservatorio Astron Brera, I-23807 Merate, Italy

来源：

X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS | 2010年 / 1248卷

关键词：

Accretion and accretion disks-black hole binaries; X-RAY-EMISSION; OUTBURST; CANDIDATES; GX-339-4; STATES; JETS;

D O I：

10.1063/1.3475157

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

I briefly outline the state-paradigm that has emerged from the study of black-hole binaries with RossiXTE. This is the starting point of a number of studies that address the connection between accretion and jet ejection and the physical nature of the hard spectral components in these systems.

引用

页码：107 / 110

页数：4

共 16 条

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[2]

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[5]

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[7] Towards a unified model for black hole X-ray binary jets [J].

Fender, RP ;

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Gallo, E .

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[8]

FENDER RP, 2009, LECT NOTES IN PRESS, V794

[9]

GALLO E, 2009, LECT NOTES IN PRESS, V794

[10]

GILFANOV M, 2009, LECT NOTES IN PRESS, V794

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