Application of the screened Coulomb potential to fit the DA-type variable star HS 0507+0434B
文献类型:期刊论文
作者 | Chen, Y. H.1,2,3 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2020-06-01 |
卷号 | 495期号:2页码:2428-2435 |
ISSN号 | 0035-8711 |
关键词 | asteroseismology: individual (HS0507+0434B) white dwarfs |
DOI | 10.1093/mnras/staa1374 |
文献子类 | Article |
英文摘要 | wdec is used to evolve grids of DA-variable (DAV) star models adopting the element diffusion scheme with pure and screened Coulomb potentials. The core compositions are thermonuclear burning results derived from mesa. mesa yields composition profiles that the version of WDEC used in this work could not accommodate (most notably, the presence of helium in the core of the model). According to the theory of rotational splitting, Fu and colleagues identified six triplets for the DAV star HS 0507 + 0434B based on 206 h of photometric data. The grids of DAV star models are used to fit the six reliable m = 0 modes. When adopting the screened Coulomb potential, a best-fitting model of log(M-He/M-*)=-3.0, log(M-H/M-*)=-6.1, T-eff = 11 790 K, M-* = 0.625M(circle dot), log g = 8.066 and sigma(RMS) = 2.08 s was obtained. Compared with adopting the pure Coulomb potential, the value of sRMS is improved by 34 per cent. This study may provide a new method for research into mode-trapping properties. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星物理学 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS关键词 | BISYSTEM OSCILLATION-THEORY ; ZZ CETI STARS ; THERMAL-CONDUCTIVITIES ; DENSE MATTER ; ASTEROSEISMOLOGY ; DIFFUSION ; EVOLUTION ; MODELS |
资助项目 | National Natural Science Foundation of China[11803004] ; National Natural Science Foundation of China[11563001] ; National Natural Science Foundation of China[11333006] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000543015800064 |
资助机构 | National Natural Science Foundation of China[11803004, 11563001, 11333006] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/23532] |
专题 | 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Chen, Y. H. |
作者单位 | 1.Institute of Astrophysics, Chuxiong Normal University, Chuxiong 675000, China 2.School of Physics and Electronical Science, Chuxiong Normal University, Chuxiong 675000, China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, PO Box 110, Kunming 650011, China |
推荐引用方式 GB/T 7714 | Chen, Y. H.. Application of the screened Coulomb potential to fit the DA-type variable star HS 0507+0434B[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,495(2):2428-2435. |
APA | Chen, Y. H..(2020).Application of the screened Coulomb potential to fit the DA-type variable star HS 0507+0434B.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,495(2),2428-2435. |
MLA | Chen, Y. H.."Application of the screened Coulomb potential to fit the DA-type variable star HS 0507+0434B".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 495.2(2020):2428-2435. |
入库方式: OAI收割
来源:云南天文台
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