NAOC Open IR
对OH/IR星演化的模型研究
何金华
2000
Source Publication云南天文台台刊
ISSN1001-7526
Volume000Issue:001Pages:71
Abstract渐近巨星分南恒星(AGB星)是一种晚期演化恒星,它是恒星作为以核反应释能为发光能源的天体的最后演化阶段。AGB星阶段的恒星具有许多有趣的性质,如很大的质量损失率(因此形成很厚的拱星尘埃气体包层),光变,热脉动(或He闪耀),强的红外超量发射,分子脉泽发射等,弄清AGB星的演化规律是研究恒星演化理论的重要任务。目前人们所知道的AGB星的演化图景是,恒星经过漫长的主序演化之后,将经过红巨星(RGB)阶
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51807
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
何金华. 对OH/IR星演化的模型研究[J]. 云南天文台台刊,2000,000(001):71.
APA 何金华.(2000).对OH/IR星演化的模型研究.云南天文台台刊,000(001),71.
MLA 何金华."对OH/IR星演化的模型研究".云南天文台台刊 000.001(2000):71.
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