A New C-D-like Diagram for SPB Stars: The Variations of Period Spacing as a Signature of Evolutionary Status
文献类型:期刊论文
作者 | Wu T(吴涛)1,2,3; Li Y(李焱)1,2,3,4; Deng ZM(邓真敏)1,2,4 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2018-11-01 |
卷号 | 867期号:1页码:13 |
ISSN号 | 0004-637X |
关键词 | asteroseismology stars: oscillations stars: interiors stars: fundamental parameters stars: individual (HD 50230, KIC 6462030, KIC 8324482, and KIC 10526294) |
DOI | 10.3847/1538-4357/aadf85 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | The slowly pulsating B-type (SPB) stars are the upper main-sequence stars on the HR diagram. Their oscillations are high-order, low-degree g-mode and can be used to probe the structure of the radiative zone near the outer boundary of the convective core and constrain the chemical mixing in stellar interiors. In SPB stars, the period spacing periodically varies with periods. It has been regarded as a signature of the chemical composition gradient beyond the convective core. Based on theoretical calculations, we find that the variation frequency of the period spacings (f(Delta P)) is related to the width of the mu-gradient region on the buoyancy radius (Lambda(mu)) with the relation of f(Delta P) similar to 0.5 Lambda(mu). This indicates that the variation frequency f(Delta P) is sensitive to the central hydrogen mass fraction X-C (i.e., the evolutionary status). Finally, we find that the variation frequency f(Delta P) and the means of the period spacings can be used to construct a new C-D-like diagram (f(Delta P) versus ), which can be used to roughly decide the stellar evolutionary stages and to approximately determine stellar mass for SPB stars. |
学科主题 | 天文学 ; 天体物理学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | GAMMA DORADUS STARS ; WHITE-DWARFS ; MODES ; ASTEROSEISMOLOGY |
资助项目 | NSFC of China[11333006] ; NSFC of China[11503076] ; NSFC of China[11773064] ; NSFC of China[11521303] ; Yunnan Applied Basic Research Projects[2017B008] ; NASA's Science Mission Directorate |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000448736000014 |
资助机构 | NSFC of China[11333006, 11503076,11773064, 11521303] ; Yunnan Applied Basic Research Projects[2017B008] ; NASA's Science Mission Directorate |
源URL | [http://ir.ynao.ac.cn/handle/114a53/18319] |
专题 | 云南天文台_恒星物理研究组 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 | Wu T(吴涛) |
作者单位 | 1.Chinese Acad Sci, Yunnan Observ, 396 Yangfangwang, Kunming 650216, Yunnan, Peoples R China 2.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, 396 Yangfangwang, Kunming 650216, Yunnan, Peoples R China 3.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
推荐引用方式 GB/T 7714 | Wu T,Li Y,Deng ZM. A New C-D-like Diagram for SPB Stars: The Variations of Period Spacing as a Signature of Evolutionary Status[J]. ASTROPHYSICAL JOURNAL,2018,867(1):13. |
APA | Wu T,Li Y,&Deng ZM.(2018).A New C-D-like Diagram for SPB Stars: The Variations of Period Spacing as a Signature of Evolutionary Status.ASTROPHYSICAL JOURNAL,867(1),13. |
MLA | Wu T,et al."A New C-D-like Diagram for SPB Stars: The Variations of Period Spacing as a Signature of Evolutionary Status".ASTROPHYSICAL JOURNAL 867.1(2018):13. |
入库方式: OAI收割
来源:云南天文台
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。