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A Note on the Supersonic Convection in Stellar Atmospheres
Xiong, Da-Run; Deng, Li-Cai
2011
Source PublicationChinese Astronomy and Astrophysics
ISSN0275-1062
Volume35Issue:4Pages:382-385
AbstractBy using a non-local convection theory, both the local and nonlocal convective envelope models of evolutionary series of stars with masses from 1 to 30 solar masses are calculated. The problem of supersonic convection is reviewed. The results show that the convective velocities in the stellar atmosphere are seriously overestimated by the local mixing-length theory. Convection is strongly supersonic in the atmospheres of yellow giant and super-giants, while the local mixing-length theory is used. However, it becomes subsonic for most stars when convection returns to the normal nonlocal treatment. Convection velocities increase with increase of luminosities of stars. There is still weak supersonic convection in few red and yellow giant and super-giants. It is suspected whether this supersonic convection in stellar atmospheres is true.
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11220
Collection院士文集_熊大闰
Recommended Citation
GB/T 7714
Xiong, Da-Run,Deng, Li-Cai. A Note on the Supersonic Convection in Stellar Atmospheres[J]. Chinese Astronomy and Astrophysics,2011,35(4):382-385.
APA Xiong, Da-Run,&Deng, Li-Cai.(2011).A Note on the Supersonic Convection in Stellar Atmospheres.Chinese Astronomy and Astrophysics,35(4),382-385.
MLA Xiong, Da-Run,et al."A Note on the Supersonic Convection in Stellar Atmospheres".Chinese Astronomy and Astrophysics 35.4(2011):382-385.
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