NAOC Open IR
一种修正的局部混合长理论
邓李才1; 熊大闰2
1999
Source Publication紫金山天文台台刊
ISSN1000-3681
Volume018Issue:003Pages:325
Abstract按照通常的局部混合长理论,在红、黄巨星和超巨星对对流区的面部将出现超声速对流。作者对此提出了质疑,并提出了一种修正的混合长公式。与传统的理论相比,对具相同质量、光度和有效温度的恒星,新理论预期一较浅的对流区,超声速对流也被有效地抑制了。其结果是在H-R图上,红超巨星支向低温方向移动了100-400K;而对中低光度恒星的结构和演化性质却没有任何可察的影响。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/48257
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.中国科学院紫金山天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
邓李才,熊大闰. 一种修正的局部混合长理论[J]. 紫金山天文台台刊,1999,018(003):325.
APA 邓李才,&熊大闰.(1999).一种修正的局部混合长理论.紫金山天文台台刊,018(003),325.
MLA 邓李才,et al."一种修正的局部混合长理论".紫金山天文台台刊 018.003(1999):325.
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