YNAO OpenIR  > 大样本恒星演化研究组
On the formation and evolution of black hole binaries
Podsiadlowski, P1; Rappaport, S2; Han ZW(韩占文)3; Podsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England.
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2003-05-11
Volume341Issue:2Pages:385-404
DOI10.1046/j.1365-8711.2003.06464.x
Contribution Rank第3完成单位
Indexed BySCI
KeywordBlack Hole Physics Gravitation Binaries : Close Stars : Individual : Cygnus X-1 Stars : Individual : Grs 1915+105 X-rays : Stars
AbstractWe 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.
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeReview
ISSN0035-8711
URL查看原文
WOS IDWOS:000182651400002
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordX-RAY BINARIES ; COMMON-ENVELOPE EVOLUTION ; LOW-MASS ; STELLAR EVOLUTION ; TIDAL CIRCULARIZATION ; VELOCITY DISTRIBUTION ; SOLAR NEIGHBORHOOD ; MAGNETIC BRAKING ; ORBITAL ELEMENTS ; OPTICAL-SPECTRUM
Citation statistics
Cited Times:175[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/4401
Collection大样本恒星演化研究组
Corresponding AuthorPodsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England.
Affiliation1.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
Recommended Citation
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.
Files in This Item:
File Name/Size DocType Version Access License
On the formation and(4885KB)期刊论文作者接受稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Podsiadlowski, P]'s Articles
[Rappaport, S]'s Articles
[Han ZW(韩占文)]'s Articles
Baidu academic
Similar articles in Baidu academic
[Podsiadlowski, P]'s Articles
[Rappaport, S]'s Articles
[Han ZW(韩占文)]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Podsiadlowski, P]'s Articles
[Rappaport, S]'s Articles
[Han ZW(韩占文)]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: On the formation and evolution of black hole binaries.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.