HL Dra: an active Algol-like binary system with a pulsating component star and a cool third body
文献类型:期刊论文
作者 | Shi XD(施相东)1,2,3,4; Qian SB(钱声帮)1,2,3,4; Li LJ(李临甲)1,3,4; Liao WP(廖文萍)1,2,3,4 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2021-08 |
卷号 | 505期号:4页码:6166-6178 |
ISSN号 | 0035-8711 |
关键词 | stars: activity stars: binaries: close stars: binaries: eclipsing stars: individual: HL Draconis stars: variables: Scuti |
DOI | 10.1093/mnras/stab1657 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | HL Draconis (HL Dra) is an oscillating eclipsing binary with an orbital period of 0.944276 d. By analysing the light curves observed with the Transiting Exoplanet Survey Satellite (TESS), it has been detected that HL Dra is an Algol-like binary system with a mass ratio of 0.361, where the radius filling factor (= r/R-L) of the primary and secondary component is 87 per cent and 98 per cent, respectively. The secondary component is almost filling its critical Roche lobe, but not entirely. The absolute parameters of the component are estimated in this paper. Both the variable O'Connell effect and the existence of superflares indicate that the secondary should have strong magnetic activities. It is discovered that the O - C curve shows a sinusoidal variation with a period of 129.88 yr. This cyclic change might be caused by the effects of the light travel time as a result of the presence of a cool red dwarf third body. The correlations between the changes of the O - C diagrams and the variable O'Connell effect during TESS observations might be caused by the magnetic activity of the secondary (i.e. the Applegate mechanism). After removal of the binary model, a total of 252 pulsation frequencies are detected from the high-precision photometric data of TESS, including 28 multiplets of tidally split frequencies. We identify two radial modes, 21 non-radial p-modes and three non-radial f-modes from the possible independent frequencies. All of these features reveal that HL Dra is a very interesting system for further investigations of binary formation and evolution, and for tidal interactions on stellar pulsations and on magnetic activities. |
学科主题 | 天文学 ; 恒星与银河系 ; 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 | ORBIT CLOSE BINARIES ; ISENTROPIC OSCILLATIONS ; TIDAL PERTURBATIONS ; ECLIPSING BINARY ; VELOCITY ; LIGHT ; PARAMETERS |
资助项目 | Chinese Natural Science FoundationNational Natural Science Foundation of China (NSFC)[11933008] ; Chinese Natural Science FoundationNational Natural Science Foundation of China (NSFC)[11873017] ; Chinese Natural Science FoundationNational Natural Science Foundation of China (NSFC)[11803084] ; NASA Office of Space ScienceNational Aeronautics & Space Administration (NASA) ; NASA Explorer ProgramNational Aeronautics & Space Administration (NASA) |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000698554000083 |
资助机构 | Chinese Natural Science FoundationNational Natural Science Foundation of China (NSFC)[11933008, 11873017, 11803084] ; NASA Office of Space ScienceNational Aeronautics & Space Administration (NASA) ; NASA Explorer ProgramNational Aeronautics & Space Administration (NASA) |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24581] |
专题 | 云南天文台_双星与变星研究组 |
通讯作者 | Shi XD(施相东) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences (CAS), PO Box 110, Kunming 650216, China; 2.University of Chinese Academy of Sciences, Yuquan Road 19, Sijingshang Block, Beijing 100049, China; 3.Key Laboratory of the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, China; 4.Center for Astronomical Mega-Science, CAS, 20A Datun Road, Chaoyang District, Beijing 100012, China |
推荐引用方式 GB/T 7714 | Shi XD,Qian SB,Li LJ,et al. HL Dra: an active Algol-like binary system with a pulsating component star and a cool third body[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,505(4):6166-6178. |
APA | Shi XD,Qian SB,Li LJ,&Liao WP.(2021).HL Dra: an active Algol-like binary system with a pulsating component star and a cool third body.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,505(4),6166-6178. |
MLA | Shi XD,et al."HL Dra: an active Algol-like binary system with a pulsating component star and a cool third body".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 505.4(2021):6166-6178. |
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。