中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
On the effect of turbulent anisotropy on pulsation stability of stars

文献类型:期刊论文

作者Zhang, Chun-Guang; Deng, Li-Cai; Xiong, Da-Run
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2017
卷号17期号:3页码:-
英文摘要Within the framework of a non- local time- dependent stellar convection theory, we study in detail the effect of turbulent anisotropy on stellar pulsation stability. The results show that anisotropy has no substantial influence on pulsation stability of g modes and low- order (radial order n(r) < 5) p modes. The effect of turbulent anisotropy increases as the radial order increases. When turbulent anisotropy is neglected, most high- order ( n(r) > 5) p modes of all low-temperature stars become unstable. Fortunately, within a wide range of the anisotropic parameter c(3), stellar pulsation stability is not sensitive to the specific value of c(3.) Therefore it is safe to say that calibration errors of the convective parameter c (3) do not cause any uncertainty in the calculation of stellar pulsation stability.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/17435]  
专题中国科学院紫金山天文台
推荐引用方式
GB/T 7714
Zhang, Chun-Guang,Deng, Li-Cai,Xiong, Da-Run. On the effect of turbulent anisotropy on pulsation stability of stars[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2017,17(3):-.
APA Zhang, Chun-Guang,Deng, Li-Cai,&Xiong, Da-Run.(2017).On the effect of turbulent anisotropy on pulsation stability of stars.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,17(3),-.
MLA Zhang, Chun-Guang,et al."On the effect of turbulent anisotropy on pulsation stability of stars".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 17.3(2017):-.

入库方式: OAI收割

来源:紫金山天文台

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