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熊大闰; 邓李才
Source Publication紫金山天文台台刊
Abstract按照通常的局部混合长理论,在红、黄巨星和超巨星对流区的顶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。
Keyword对流 恒星演化 超巨星 晚型星
Subject Area天文和天体物理
Document Type期刊论文
Recommended Citation
GB/T 7714
熊大闰,邓李才. 一种修正的局部混合长理论[J]. 紫金山天文台台刊,1999,0(3):5.
APA 熊大闰,&邓李才.(1999).一种修正的局部混合长理论.紫金山天文台台刊,0(3),5.
MLA 熊大闰,et al."一种修正的局部混合长理论".紫金山天文台台刊 0.3(1999):5.
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