中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
New extended atomic data in cool star model atmospheres Using Kurucz's new iron data in MAFAGS-OS models

文献类型:期刊论文

作者Grupp, F.1,2; Kurucz, R. L.3; Tan, K.4
刊名ASTRONOMY & ASTROPHYSICS
出版日期2009-08-01
卷号503期号:1页码:177-181
关键词atomic data Sun: abundances stars: abundances stars: atmospheres stars: fundamental parameters stars: late-type
英文摘要Context. Cool star model atmospheres are a common tool for the investigation of stellar masses, ages and elemental abundance composition. Theoretical atmospheric models strongly depend on the atomic data used when calculating them.
收录类别SCI
语种英语
WOS记录号WOS:000269150300020
源URL[http://ir.bao.ac.cn/handle/114a11/7558]  
专题国家天文台_光学天文研究部
作者单位1.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
2.Univ Sternwarte, D-81679 Munich, Germany
3.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
4.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Grupp, F.,Kurucz, R. L.,Tan, K.. New extended atomic data in cool star model atmospheres Using Kurucz's new iron data in MAFAGS-OS models[J]. ASTRONOMY & ASTROPHYSICS,2009,503(1):177-181.
APA Grupp, F.,Kurucz, R. L.,&Tan, K..(2009).New extended atomic data in cool star model atmospheres Using Kurucz's new iron data in MAFAGS-OS models.ASTRONOMY & ASTROPHYSICS,503(1),177-181.
MLA Grupp, F.,et al."New extended atomic data in cool star model atmospheres Using Kurucz's new iron data in MAFAGS-OS models".ASTRONOMY & ASTROPHYSICS 503.1(2009):177-181.

入库方式: OAI收割

来源:国家天文台

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