On the formation and evolution of black hole binaries

doi:10.1046/j.1365-8711.2003.06464.x

YNAO OpenIR > 大样本恒星演化研究组

	On the formation and evolution of black hole binaries
	Podsiadlowski, P 1; Rappaport, S 2; Han ZW(韩占文)3 ; Podsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England.
发表期刊	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2003-05-11
卷号	341 期号:2 页码:385-404
DOI	10.1046/j.1365-8711.2003.06464.x
产权排序	第3完成单位
收录类别	SCI
关键词	Black Hole Physics Gravitation Binaries : Close Stars : Individual : Cygnus X-1 Stars : Individual : Grs 1915+105 X-rays : Stars
摘要	We present the results of a systematic study of the formation and evolution of binaries containing black holes and normal-star companions with a wide range of masses. We first reexamine the standard formation scenario for close black hole binaries, where the progenitor system, a binary with at least one massive component, experienced a common-envelope phase and where the spiral-in of the companion in the envelope of the massive star caused the ejection of the envelope. We estimate the formation rates for different companion masses and different assumptions about the common-envelope structure and other model parameters. We find that black hole binaries with intermediate- and high-mass secondaries can form for a wide range of assumptions, while black hole binaries with low-mass secondaries can only form with apparently unrealistic assumptions (in agreement with previous studies). We then present detailed binary evolution sequences for black hole binaries with secondaries of 2 to 17 M(circle dot) and demonstrate that in these systems the black hole can accrete appreciably even if accretion is Eddington-limited (up to 7 M(circle dot) for an initial black hole mass of 10 M(circle dot) ) and that the black holes can be spun up significantly in the process. We discuss the implications of these calculations for well-studied black hole binaries (in particular GRS 1915+105) and ultraluminous X-ray sources of which GRS 1915+105 appears to represent a typical Galactic counterpart. We also present a detailed evolutionary model for Cygnus X-1, a massive black hole binary, which suggests that at present the system is most likely in a wind mass-transfer phase following an earlier Roche-lobe overflow phase. Finally, we discuss how some of the assumptions in the standard model could be relaxed to allow the formation of low-mass, short-period black hole binaries, which appear to be very abundant in nature.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Review
ISSN	0035-8711
URL	查看原文
WOS记录号	WOS:000182651400002
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	X-RAY BINARIES ; COMMON-ENVELOPE EVOLUTION ; LOW-MASS ; STELLAR EVOLUTION ; TIDAL CIRCULARIZATION ; VELOCITY DISTRIBUTION ; SOLAR NEIGHBORHOOD ; MAGNETIC BRAKING ; ORBITAL ELEMENTS ; OPTICAL-SPECTRUM
引用统计	被引频次：259[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/4401
专题	大样本恒星演化研究组
通讯作者	Podsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England.
作者单位	1.University of Oxford, Department of Astrophysics, Oxford OX1 3RH 2.Department of Physics and Centre for Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 3.Yunnan Observatory, National Astronomical Observatories, the Chinese Academy of Sciences, Kunming 650011, China
推荐引用方式 GB/T 7714	Podsiadlowski, P,Rappaport, S,Han ZW,et al. On the formation and evolution of black hole binaries[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2003,341(2):385-404.
APA	Podsiadlowski, P,Rappaport, S,Han ZW,&Podsiadlowski, P .(2003).On the formation and evolution of black hole binaries.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,341(2),385-404.
MLA	Podsiadlowski, P,et al."On the formation and evolution of black hole binaries".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 341.2(2003):385-404.

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