相接双星的结构和演化研究
发布时间：2022-08-11 10:14
利用Huang等人基于Kippenhann的相接双星模型开发的程序,计算了初始周期为P0=2.772d和P0=1.808d的两个系统的演化轨迹,并对后者相接状态的演化进行了初步探究.
【文章页数】：3 页
【文章目录】：
1 引言
2 相接双星演化的数值模拟
2.1 系统A的演化轨迹模拟
2.2 系统B的演化轨迹模拟
3 结束语
【参考文献】：
期刊论文
[1]A Model for Contact Binary Systems[J]. Han-Feng Song1,2, Run-Qian Huang1 and Shao-Lan Bi1 1 National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011; 2 Graduate School of Chinese Academy of Sciences, Beijing 100049. Chinese Journal of Astronomy and Astrophysics. 2007(04)
[2]On the Physical Processes in Contact Binary Systems[J]. Run-Qian Huang1, Han-Feng Song1,2 and Shao-Lan Bi1 1 National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011;2 Graduate University of Chinese Academy of Sciences, Beijing 100049. Chinese Journal of Astronomy and Astrophysics. 2007(02)
本文编号：3674470
【文章页数】：3 页
【文章目录】：
1 引言
2 相接双星演化的数值模拟
2.1 系统A的演化轨迹模拟
2.2 系统B的演化轨迹模拟
3 结束语
【参考文献】：
期刊论文
[1]A Model for Contact Binary Systems[J]. Han-Feng Song1,2, Run-Qian Huang1 and Shao-Lan Bi1 1 National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011; 2 Graduate School of Chinese Academy of Sciences, Beijing 100049. Chinese Journal of Astronomy and Astrophysics. 2007(04)
[2]On the Physical Processes in Contact Binary Systems[J]. Run-Qian Huang1, Han-Feng Song1,2 and Shao-Lan Bi1 1 National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011;2 Graduate University of Chinese Academy of Sciences, Beijing 100049. Chinese Journal of Astronomy and Astrophysics. 2007(02)
本文编号：3674470
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