Calibrating the alpha parameter of convective efficiency using observed stellar properties

	Calibrating the alpha parameter of convective efficiency using observed stellar properties
	Wu, X. S.1,2,3; Alexeeva, S.4; Mashonkina, L.4; Wang, L.1,2; Zhao, G.1 ; Grupp, F.2,5
刊名	ASTRONOMY & ASTROPHYSICS
	2015-05-01
卷号	577
关键词	stars: fundamental parameters stars: atmospheres stars: late-type
英文摘要	Context. Synthetic model atmosphere calculations are still the most commonly used tool when determining precise stellar parameters and stellar chemical compositions. Besides three-dimensional models that consistently solve for hydrodynamic processes, one-dimensional models that use an approximation for convective energy transport play the major role.
收录类别	SCI
语种	英语
WOS记录号	WOS:000357345900086
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/5660]
专题	国家天文台_光学天文研究部
作者单位	1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 2.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany 3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 4.Russian Acad Sci, Inst Astron, Moscow 119017, Russia 5.Univ Sternwarte, D-81679 Munich, Germany
推荐引用方式 GB/T 7714	Wu, X. S.,Alexeeva, S.,Mashonkina, L.,et al. Calibrating the alpha parameter of convective efficiency using observed stellar properties[J]. ASTRONOMY & ASTROPHYSICS,2015,577.
APA	Wu, X. S.,Alexeeva, S.,Mashonkina, L.,Wang, L.,Zhao, G.,&Grupp, F..(2015).Calibrating the alpha parameter of convective efficiency using observed stellar properties.ASTRONOMY & ASTROPHYSICS,577.
MLA	Wu, X. S.,et al."Calibrating the alpha parameter of convective efficiency using observed stellar properties".ASTRONOMY & ASTROPHYSICS 577(2015).