YNAO OpenIR  > 大样本恒星演化研究组
Common envelope evolution: where we stand and how we can move forward
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; Lu, G12,13; Marsh, T14; Podsiadlowski, P15; Potter, A16; Soker, N17; Taam, R8,18; Tauris, TM19,20; van den Heuvel, EPJ; Webbink, RF; Ivanova, N (reprint author), Univ Alberta, Dept Phys, Edmonton, AB T6G 3E1, Canada.
Contribution Rank第4完成单位
Indexed BySCI ; EI
KeywordClose Binaries Stellar Structure Interiors Evolution Hydrodynamics
AbstractThis 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.
Funding OrganizationNational Science Foundation [NSF PHY05-51164] ; Kavli Foundation, NSFC [10903001, 11250110055] ; Chinese Academy of Sciences [KJCX2-YW-T24] ; NSFC [10973036, 11173055, 11033008, 11203065, 10873008] ; Yunnan National Science Foundation [2008CD155] ; National Nuclear Security Administration of the US Department of Energy at Los Alamos National Laboratory ; National Basic Research Program of China (973 Program) [2009CB824800] ; STFC ; NSF [AST-0703950] ; Leids Kerkhoven-Bosscha Fonds ; Department of Astronomy, University of Illinois at Urbana-Champaign ; [DE-AC52-06NA25396]
Subject AreaAstronomy & Astrophysics
WOS IDWOS:000323907900001
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
Citation statistics
Cited Times:265[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Corresponding AuthorIvanova, N (reprint author), Univ Alberta, Dept Phys, Edmonton, AB T6G 3E1, Canada.
Affiliation1.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
11.Department of Astronomy and Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing, 210093, China
12.National Astronomical Observatories/Urumqi Observatory, The Chinese Academy of Sciences, Urumqi, 830011, China
13.School of Physics, Xinjiang University, Urumqi, 830046, China
14.Department of Physics, University of Warwick, Coventry, CV4 7AL, UK
15.Sub-Department of Astronomy, Oxford University, Oxford, OX1 3RH, UK
16.Institute of Astronomy, University of Cambridge, The Observatories, Madingley Road, Cambridge, CB3 0HA, UK
17.Department of Physics, Technion, Israel Institute of Technology, Haifa, 32000, Israel
18.Academia Sinica Institute of Astrophysics and Astronomy-TIARA, P.O. Box 23-141, Taipei, 10617, Taiwan
19.Argelander-Insitut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany
20.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121, Bonn, Germany
Recommended Citation
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.,...&Ivanova, N .(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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