Accretion disc atmospheres and winds in low-mass X-ray binaries

被引：91
|
作者：
Trigo, M. Diaz [1 ]
Boirin, L. [2 ]
机构：
[1] ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[2] Univ Strasbourg, Observ Astronom Strasbourg, CNRS, UMR 7550, 11 Rue Univ, F-67000 Strasbourg, France
来源：
ASTRONOMISCHE NACHRICHTEN | 2016年 / 337卷 / 4-5期
关键词：
accretion; accretion disks; black hole physics; stars: neutron; techniques: spectroscopy; X-rays: binaries; TRANSMISSION GRATING SPECTROMETER; ABSORPTION-LINE FEATURES; BLACK-HOLE CANDIDATE; XMM-NEWTON OBSERVATIONS; PULSAR IGR J17480-2446; COMPTON-HEATED WINDS; SOURCE GRO J1655-40; FE K ABSORPTION; CHANDRA OBSERVATION; CIRCINUS X-1;
D O I：
10.1002/asna.201612315
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In the last decade, X-ray spectroscopy has enabled a wealth of discoveries of photoionised absorbers in X-ray binaries. Studies of such accretion disc atmospheres and winds are of fundamental importance to understand accretion processes and possible feedback mechanisms to the environment. In this work, we review the current observational state and theoretical understanding of accretion disc atmospheres and winds in low-mass X-ray binaries, focusing on the wind launching mechanisms and on the dependence on accretion state. We conclude with issues that deserve particular attention. (C) 2016 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim
引用
收藏
页码：368 / 374
页数：7
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