|
|||||
|
|
| 双星演化与大样本恒星演化 | |
| 引用本文： | 韩占文,Eggleton P P,Tout C A,Webbink R F. 双星演化与大样本恒星演化[J]. 天文学进展, 2001, 19(2): 242-245 |
| 作者姓名： | 韩占文 Eggleton P P Tout C A Webbink R F |
| 作者单位： | 1. 中国科学院云南天文台 2. IGPP,Lawrence Livermore National Laboratory, 3. Astrophysics,NAPL,Oxford University, 4. Institute of Astronomy,University of Cambridge, 5. Department of Astronomy,University of Illinois at Urbana-Champaign, |
| 摘 要： | 主要介绍了大样本恒星演化所面临的困难，为解决困难所做的努力及对未来的展望。 |
| 关 键 词： | 恒星演化 双星演化 星族合成 形成机制 |
| 修稿时间： | 2000-12-14 |
Binary Evolution and Binary Population Synthesis |
|
| Han Zhanwen. Binary Evolution and Binary Population Synthesis[J]. Progress In Astronomy, 2001, 19(2): 242-245 | |
| Authors: | Han Zhanwen |
| Abstract: | The purpose of binary population synthesis is to detechne, as far as possible, the consistency of our theoretical understanding of single and binary stars with the statistics of stars in our galaxy (and ultimately other galaxies). It is important to fit all types of stellar systems simulta- neously rather than just concentrsting on particular irces of stars. In this paper, we describe the difficulties and problems of binary populstion synthesis, and the efforts we have made to establish a self-consistent binary population synthesis model. |
| Keywords: | stars-stellar evolution-binary evolution-binary population synthesis |
| 本文献已被 CNKI 维普 万方数据 等数据库收录！ | |