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Common envelope evolution: where we stand and how we can move forward

文献类型：期刊论文

作者Ivanova, N1; Justham, S2,3; Chen XF(陈雪飞)4,5; De Marco, O6; Fryer, CL7; Gaburov, E8; Ge HW(葛宏伟)4,5; Glebbeek, E9,10; Han ZW(韩占文)4,5; Li, XD11
刊名ASTRONOMY AND ASTROPHYSICS REVIEW
出版日期2013-02-27
卷号21
关键词Close binaries Stellar structure interiors evolution Hydrodynamics
ISSN号0935-4956
产权排序第四完成单位
通讯作者Ivanova, N (reprint author), Univ Alberta, Dept Phys, Edmonton, AB T6G 3E1, Canada.
英文摘要This work aims to present our current best physical understanding of common-envelope evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas which should point the way forward for progress in this important but long-standing and largely unconquered problem. Unusually for CEE-related work, we mostly try to avoid relying on results from population synthesis or observations, in order to avoid potentially being misled by previous misunderstandings. As far as possible we debate all the relevant issues starting from physics alone, all the way from the evolution of the binary system immediately before CEE begins to the processes which might occur just after the ejection of the envelope. In particular, we include extensive discussion about the energy sources and sinks operating in CEE, and hence examine the foundations of the standard energy formalism. Special attention is also given to comparing the results of hydrodynamic simulations from different groups and to discussing the potential effect of initial conditions on the differences in the outcomes. We compare current numerical techniques for the problem of CEE and also whether more appropriate tools could and should be produced (including new formulations of computational hydrodynamics, and attempts to include 3D processes within 1D codes). Finally we explore new ways to link CEE with observations. We compare previous simulations of CEE to the recent outburst from V1309 Sco, and discuss to what extent post-common-envelope binaries and nebulae can provide information, e.g. from binary eccentricities, which is not currently being fully exploited.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]X-RAY BINARIES ; SMOOTHED PARTICLE HYDRODYNAMICS ; DOUBLE-CORE EVOLUTION ; BLACK-HOLE BINARIES ; DOUBLE WHITE-DWARFS ; SUBDWARF-B-STARS ; SHAPING PLANETARY-NEBULAE ; DEGENERATE NEUTRON CORES ; BINDING-ENERGY PARAMETER ; ASYMPTOTIC GIANT BRANCH
收录类别SCI ; EI
原文出处http://link.springer.com/article/10.1007%2Fs00159-013-0059-2
语种英语
WOS记录号WOS:000323907900001
源URL[http://ir.ynao.ac.cn/handle/114a53/4560]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Physics Department, University of Alberta, Edmonton, AB, T6G 3E1, Canada
2.National Astronomical Observatories, The Chinese Academy of Sciences, Beijing, China
3.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871, China
4.National Astronomical Observatories/Yunnan Observatory, The Chinese Academy of Sciences, Kunming, 650011, China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, The Chinese Academy of Sciences, Kunming, 650011, China
6.Department of Physics & Astronomy, Macquarie University, Sydney, NSW, 2109, Australia
7.Computational Science Division, Los Alamos National Laboratory, CCS-2, MS D409, Los Alamos, NM, 87545, USA
8.Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) & Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Rd, Evanston, IL, 60208, USA
9.Department of Physics & Astronomy, McMaster University, 1280 Main Street West, Hamilton, Ontario, L8S 4M1, Canada
10.Department of Astrophysics/IMAPP, Radboud University, P.O. Box 9010, Nijmegen, The Netherlands
推荐引用方式
GB/T 7714		 Ivanova, N,Justham, S,Chen XF,et al. Common envelope evolution: where we stand and how we can move forward[J]. ASTRONOMY AND ASTROPHYSICS REVIEW,2013,21.
APA Ivanova, N.,Justham, S.,Chen XF.,De Marco, O.,Fryer, CL.,...&Webbink, RF.(2013).Common envelope evolution: where we stand and how we can move forward.ASTRONOMY AND ASTROPHYSICS REVIEW,21.
MLA Ivanova, N,et al."Common envelope evolution: where we stand and how we can move forward".ASTRONOMY AND ASTROPHYSICS REVIEW 21(2013).

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来源：云南天文台

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