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Beryllium depletion in the solar atmosphere
Xiong, DR; Deng, LC
2003
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
ISSN0275-1062
Volume27Issue:1Pages:1-3
AbstractUsing a non-local convection theory for chemically inhomogeneous stars, the beryllium depletion of the Sun is calculated. The results show that Be is slightly depleted(similar to5%) in the evolutionary model for the Sun.
KeywordSun : Abundances Stars : Abundances Convection
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordLITHIUM ABUNDANCE GAP ; SEQUENCE MASS-LOSS ; MAIN-SEQUENCE ; STELLAR MODELS ; F-STARS ; DIFFUSION ; CIRCULATION ; SUN
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000181305100001
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11197
Collection院士文集_熊大闰
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Xiong, DR,Deng, LC. Beryllium depletion in the solar atmosphere[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2003,27(1):1-3.
APA Xiong, DR,&Deng, LC.(2003).Beryllium depletion in the solar atmosphere.CHINESE ASTRONOMY AND ASTROPHYSICS,27(1),1-3.
MLA Xiong, DR,et al."Beryllium depletion in the solar atmosphere".CHINESE ASTRONOMY AND ASTROPHYSICS 27.1(2003):1-3.
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