Solar-like and Mira-like oscillations of stars - A uniform excitation mechanism
文献类型：期刊论文
| 作者 | Xiong, Da-Run1 ; Deng, Li-Cai2
|
| 刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2013-11-01 |
| 卷号 | 13期号:11页码:1269-1294 |
| 关键词 | convection stars: oscillations stars: late-type stars: evolution |
| ISSN号 | 0035-8711 |
| 通讯作者 | Zhang, XG (通讯作者) Chinese Acad Sci, Purple Mt Observ, 2 Beijing XiLu, Nanjing 210008, Jiangsu, Peoples R China. |
| 英文摘要 | Using a non-local and time-dependent theory of convection, we have calculated the linear non-adiabatic oscillations of the radial and low-degree F-p39 modes for evolutionary models from the main sequence to the asymptotic giant branch for stars with solar abundance (X = 0. 7 0, Z = 0. 0 2) in the mass range of 0.6-3.0 M circle dot. The results show that low luminosity cool stars tend to be solar-like oscillators, whose low-order modes are stable, but intermediate and high order p-modes are pulsationally unstable; their unstable modes have a wide range in frequency and small values for amplitude growth rates. For stars with increasing luminosity and therefore lower temperature, the unstable modes shift towards lower orders, the corresponding range of frequency decreases, and the amplitude growth rate increases. High luminosity red giant stars behave like typical Mira-like oscillators. The effects of the coupling between convection and oscillations on pulsational instability have been carefully analyzed in this work. Our research shows that convection does not simply act as a damping mechanism for oscillations, and the complex nature of the coupling between convection and oscillations makes turbulent convection sometimes behave as damping, and sometimes as excitation. Such a picture can not only naturally account for the red edge of the instability strip, but also the solar-like oscillations in low luminosity red stars and Mira-like ones in high luminosity red giants. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | MIXING-LENGTH THEORY ; RED GIANTS ; P-MODES ; STOCHASTIC EXCITATION ; NONADIABATIC OSCILLATIONS ; 5-MINUTE OSCILLATIONS ; TURBULENT CONVECTION ; NONLOCAL CONVECTION ; PULSATING STARS ; ACOUSTIC MODES |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000326281500001 |
| 公开日期 | 2014-01-08 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/9921]  |
| 专题 | 紫金山天文台_南极天文中心 |
| 作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Xiong, Da-Run,Deng, Li-Cai. Solar-like and Mira-like oscillations of stars - A uniform excitation mechanism[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2013,13(11):1269-1294. |
| APA | Xiong, Da-Run,&Deng, Li-Cai.(2013).Solar-like and Mira-like oscillations of stars - A uniform excitation mechanism.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,13(11),1269-1294. |
| MLA | Xiong, Da-Run,et al."Solar-like and Mira-like oscillations of stars - A uniform excitation mechanism".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 13.11(2013):1269-1294. |
入库方式： OAI收割
来源：紫金山天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。