The Nature of the Accretion Flow in the Low-hard State

被引：1

作者：

Reynolds, Mark T. ^{[1
]}

Miller, Jon M. ^{[1
]}

机构：

[1] Univ Michigan, Dept Astron, Ann Arbor, MI 48103 USA

来源：

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

关键词：

accretion; accretion discs; black hole physics; X-rays: binaries; INNER COOL DISKS; LOW/HARD STATE; BLACK-HOLES; REFLECTION; CYGNUS-X-1; MASS;

D O I：

10.1063/1.3475199

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations over the past number of years have cast significant doubt on the current paradigm describing the geometry of the accretion flow in the low-hard state. Here, we summarize the relevant observations in addition to a number of new Suzaku observations and discuss their implications for the geometry of the accretion flow in the low-hard state.

引用

页码：191 / 192

页数：2

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