ontheeffectofturbulentanisotropyonpulsationstabilityofstars
文献类型:期刊论文
作者 | Zhang Chunguang1; Deng Licai1; Xiong Darun2![]() |
刊名 | researchinastronomyandastrophysics
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出版日期 | 2017 |
卷号 | 17期号:3页码:10 |
ISSN号 | 1674-4527 |
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 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/332002/31171] ![]() |
专题 | 中国科学院紫金山天文台 |
作者单位 | 1.中国科学院国家天文台 2.中国科学院紫金山天文台 |
推荐引用方式 GB/T 7714 | Zhang Chunguang,Deng Licai,Xiong Darun. ontheeffectofturbulentanisotropyonpulsationstabilityofstars[J]. researchinastronomyandastrophysics,2017,17(3):10. |
APA | Zhang Chunguang,Deng Licai,&Xiong Darun.(2017).ontheeffectofturbulentanisotropyonpulsationstabilityofstars.researchinastronomyandastrophysics,17(3),10. |
MLA | Zhang Chunguang,et al."ontheeffectofturbulentanisotropyonpulsationstabilityofstars".researchinastronomyandastrophysics 17.3(2017):10. |
入库方式: OAI收割
来源:紫金山天文台
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