NAOC Open IR
关于恒星大气超声对流的注释
熊大闰1; 邓李才2
2011
Source Publication天文学报
ISSN0001-5245
Volume052Issue:003Pages:177
Abstract1引言 尽管有诸多的不满之处,由于其物理上的直观性和应用上的简单性,至今混合长理论仍几乎是唯一一个广泛用于恒星结构、演化和脉动计算的恒星对流理论.混合长理论预言,在红、黄巨星和超巨星大气中,对流是超声速的.我们曾指出,
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51468
Collection中国科学院国家天文台
Affiliation1.中国科学院紫金山天文台
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
熊大闰,邓李才. 关于恒星大气超声对流的注释[J]. 天文学报,2011,052(003):177.
APA 熊大闰,&邓李才.(2011).关于恒星大气超声对流的注释.天文学报,052(003),177.
MLA 熊大闰,et al."关于恒星大气超声对流的注释".天文学报 052.003(2011):177.
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