期刊
ASTRONOMY & ASTROPHYSICS
卷 389, 期 2, 页码 478-484出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20020600
关键词
stars : dwarf novae; stars : novae, cataclysmic variables; stars : variables : general
The long-term visual light curve parameters of 36 dwarf novae are measured. The data is anayzed in search of likely relationships among the light curve parameters and system parameters. New relations of the orbital period with the mean light curve parameters are given. Our findings for the correlation analysis of individual systems agree with some of the results in previous studies. Almost all of the systems in this study have a bimodal frequency distribution of the outburst duration. By comparing the observational correlations with their theoretical counterparts, we find that the value of the viscosity parameter of the disk instability model is alpha(hot) approximate to 0.2.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据