| A self-consistent binary population synthesis model | |
Han ZW(韩占文)1 ; Eggleton, PP2; Podsiadlowski, P3; Tout, CA2; Webbink, RF4
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| 会议录名称 | ASTRONOMICAL SOCIETY OF THE PACIFIC (ASP) CONFERENCE SERIES - EVOLUTION OF BINARY AND MULTIPLE STAR SYSTEMS: A MEETING IN CELEBRATION OF PETER EGGLETON'S 60TH BIRTHDAY |
| 2001 | |
| 卷号 | 229 |
| 页码 | 205-216 |
| 会议录编者/会议主办者 | Podsiadlowski, P; Rappaport, S; King, A; DAntona, F; Burderi, L |
| 产权排序 | 第1完成单位 |
| 收录类别 | CPCI |
| 会议名称 | Conference on Evolution of Binary and Multiple Star Systems |
| 会议日期 | 2000-06-25 |
| 会议地点 | BORMIO, ITALY |
| 会议赞助商 | Osservatorio Astronomico Roma; Lawrence Livermore Natl Lab |
| 摘要 | Binary population synthesis (BPS) is an algorithm to evolve millions of stars (including binaries) simultaneously. It plays an important role in the theory of stellar evolution and is potentially important in the study of galaxies. Previous studies of BPS employed different assumptions in the explanations of different objects, and sometimes adopted non-physical model parameters. We try to establish a self-consistent BPS model in order to explain many objects in a self-consistent way and to avoid unnatural model parameters. We present the model and some preliminary results in this paper. |
| 项目资助者 | N/A |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 恒星与银河系 |
| 文章类型 | Proceedings Paper |
| 出版者 | ASTRONOMICAL SOC PACIFIC |
| 出版地 | 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA |
| ISBN号 | 1-58381-061-7 |
| URL | 查看原文 |
| 归档日期 | 2001-08-09 |
| WOS记录号 | WOS:000176235800020 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | X-ray Binaries ; Mass-ratio Distribution ; Double White-dwarfs ; Planetary-nebulae ; Spectroscopic Binaries ; Cataclysmic Variables ; Stellar Evolution ; Close Binaries ; Space Density ; Short-period |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/219 |
| 专题 | 大样本恒星演化研究组 |
| 通讯作者 | Han ZW(韩占文) |
| 作者单位 | 1.Yunnan Observatory, Academia Sinica, Kunming, 650011, P. R. China 2.Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK 3.Oxford University, Oxford, OX1 3RH, UK 4.Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801, USA |
| 第一作者单位 | 中国科学院云南天文台 |
| 通讯作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Han ZW,Eggleton, PP,Podsiadlowski, P,et al. A self-consistent binary population synthesis model[C]//Podsiadlowski, P; Rappaport, S; King, A; DAntona, F; Burderi, L. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2001:205-216. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| A Self-Consistent Bi（976KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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