YNAO OpenIR  > 恒星物理研究组
TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076
Jiang, Chen1; Bedding, Timothy R.2,3; Stassun, Keivan G.4,5; Veras, Dimitri6,7; Corsaro, Enrico8; Buzasi, Derek L.9; Miko?ajczyk,Przemys?aw10; Zhang QS(张钱生)11,12,13,14; Ou, Jian-wen1; Campante, Tiago L.15,16; Rodrigues, Thaíise S.17; Nsamba, Benard15,18; Bossini, Diego15; Kane, Stephen R.19; Joel Ong, Jia Mian20; Y?ld?z, Mutlu21; ?elik Orhan, Zeynep21; ?rtel, Sibel21; Wu T(吴涛)22,23,24; Zhang XY(张昕旖)22,23,25; Li, Tanda2,3,26; Basu, Sarbani20; Cunha, Margarida S.15,16,26; Christensen-Dalsgaard, J?rgen3; Chaplin, William J.3,26
发表期刊The Astrophysical Journal
2020-06-01
卷号896期号:1页码:10
DOI10.3847/1538-4357/ab8f29
产权排序第22完成单位
收录类别SCI
关键词Asteroseismology Exoplanet systems
摘要

The Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission aiming to search for exoplanets that transit bright stars. The high-quality photometric data of TESS are excellent for the asteroseismic study of solar-like stars. In this work, we present an asteroseismic analysis of the red-giant star HD?222076 hosting a long-period (2.4 yr) giant planet discovered through radial velocities. Solar-like oscillations of HD?222076 are detected around 203 μHz by TESS for the first time. Asteroseismic modeling, using global asteroseismic parameters as inputs, yields a determination of the stellar mass ( ), radius ( ), and age (7.4?±?2.7 Gyr), with precisions greatly improved from previous studies. The period spacing of the dipolar mixed modes extracted from the observed power spectrum reveals that the star is on the red-giant branch burning hydrogen in a shell surrounding the core. We find that the planet will not escape the tidal pull of the star and will be engulfed into it within about 800 Myr, before the tip of the red-giant branch is reached.

资助项目Strategic Priority Research Program of the Chinese Academy of Sciences[XDB 41000000] ; National Key Program for Science and Technology Research and Development[2017YFB0203300] ; NASA Explorer Program ; ESA PRODEX[PEA 4000119301] ; Stellar Astrophysics Centre (SAC) - Danish National Research Foundation[DNRF106] ; Fundamental Research Funds for the Central Universities[19lgpy278] ; National Natural Science Foundation of China[11303087] ; Ten Thousand Talents Program of Yunnan Province ; Chinese Academy of Sciences (Light of West China Program, Youth Innovation Promotion Association) ; STFC via an Ernest Rutherford Fellowship[ST/P003850/1] ; NSFC of China[11503076] ; NSFC of China[11773064] ; NSFC of China[11873084] ; NSFC of China[11521303] ; Yunnan Applied Basic Research Projects[2017B008] ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Whitaker Center for STEM Education at Florida Gulf Coast University ; Alexander von Humboldt Foundation at the Max-Planck-Institut fur Astrophysik (MPA) ; Australian Research Council[DE 180101104] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (CartographY)[804752] ; NCN[2016/21/B/ST9/01126] ; Scientific and Technological Research Council of Turkey[TUBITAK:118F352] ; European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant[792848] ; FCT-Fundacao para a Ciencia e a Tecnologia[UIDB/04434/2020] ; FCT-Fundacao para a Ciencia e a Tecnologia[UIDP/04434/2020] ; FCT-Fundacao para a Ciencia e a Tecnologia[PTDC/FIS-AST/30389/2017] ; FEDER-Fundo Europeu de Desenvolvimento Regional through COMPETE2020 - Programa Operacional Competitividade e Internacionalizacao[POCI-01-0145-FEDER-030389]
项目资助者Strategic Priority Research Program of the Chinese Academy of Sciences[XDB 41000000] ; National Key Program for Science and Technology Research and Development[2017YFB0203300] ; NASA Explorer Program ; ESA PRODEX[PEA 4000119301] ; Stellar Astrophysics Centre (SAC) - Danish National Research Foundation[DNRF106] ; Fundamental Research Funds for the Central Universities[19lgpy278] ; National Natural Science Foundation of China[11303087] ; Ten Thousand Talents Program of Yunnan Province ; Chinese Academy of Sciences (Light of West China Program, Youth Innovation Promotion Association) ; STFC via an Ernest Rutherford Fellowship[ST/P003850/1] ; NSFC of China[11503076, 11773064, 11873084, 11521303] ; Yunnan Applied Basic Research Projects[2017B008] ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; Whitaker Center for STEM Education at Florida Gulf Coast University ; Alexander von Humboldt Foundation at the Max-Planck-Institut fur Astrophysik (MPA) ; Australian Research Council[DE 180101104] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (CartographY)[804752] ; NCN[2016/21/B/ST9/01126] ; Scientific and Technological Research Council of Turkey[TUBITAK:118F352] ; European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant[792848] ; FCT-Fundacao para a Ciencia e a Tecnologia[UIDB/04434/2020, UIDP/04434/2020, PTDC/FIS-AST/30389/2017] ; FEDER-Fundo Europeu de Desenvolvimento Regional through COMPETE2020 - Programa Operacional Competitividade e Internacionalizacao[POCI-01-0145-FEDER-030389]
语种英语
学科领域天文学 ; 恒星与银河系
文章类型Article
出版者IOP PUBLISHING LTD
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号IOP:0004-637X-896-1-ab8f29
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR-LIKE OSCILLATIONS ; KEPLER ; PLANETS ; COMPANIONS ; RADIATION ; GIANTS ; MASSES ; RADII ; TIME
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/23448
专题恒星物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Jiang, Chen
作者单位1.School of Physics and Astronomy, Sun Yat-Sen University, No. 135, Xingang Xi Road, Guangzhou, 510275, People's Republic of China
2.Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
3.Stellar Astrophysics Centre (SAC), Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
4.Vanderbilt University, Department of Physics and Astronomy, 6301 Stevenson Center Ln., Nashville, TN 37235, USA
5.Vanderbilt Initiative in Data-intensive Astrophysics (VIDA), 6301 Stevenson Center Ln., Nashville, TN 37235, USA
6.Centre for Exoplanets and Habitability, University of Warwick, Coventry CV4 7AL, UK
7.Department of Physics, University of Warwick, Coventry CV4 7AL, UK
8.INAF—Osservatorio Astrofisico di Catania, via S. Sofia 78, I-95123 Catania, Italy
9.Department of Chemistry & Physics, Florida Gulf Coast University, 10501 FGCU Boulevard S., Fort Myers, FL 33965, USA
10.Astronomical Institute, University of Wroc?aw, Miko?aja Kopernika 11, 51-622 Wroc?aw, Poland
11.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China
12.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China
13.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China
14.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
15.Instituto de Astrofísica e Ciências do Espa?o, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
16.Departamento de Física e Astronomia, Faculdade de Ciências da Universidade do Porto, Rua do Campo Alegre, s/n, 4169-007 Porto, Portugal
17.Osservatorio Astronomico di Padova—INAF, Vicolo dellOsservatorio 5, I-35122 Padova, Italy
18.Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching, Germany
19.Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA
20.Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA
21.Department of Astronomy and Space Sciences, Science Faculty, Ege University, 35100, Bornova, ?zmir, Turkey
22.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China
23.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China
24.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China
25.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
26.School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, UK
推荐引用方式
GB/T 7714
Jiang, Chen,Bedding, Timothy R.,Stassun, Keivan G.,et al. TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076[J]. The Astrophysical Journal,2020,896(1):10.
APA Jiang, Chen.,Bedding, Timothy R..,Stassun, Keivan G..,Veras, Dimitri.,Corsaro, Enrico.,...&Chaplin, William J..(2020).TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076.The Astrophysical Journal,896(1),10.
MLA Jiang, Chen,et al."TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076".The Astrophysical Journal 896.1(2020):10.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
TESS Asteroseismic A(2713KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Jiang, Chen]的文章
[Bedding, Timothy R.]的文章
[Stassun, Keivan G.]的文章
百度学术
百度学术中相似的文章
[Jiang, Chen]的文章
[Bedding, Timothy R.]的文章
[Stassun, Keivan G.]的文章
必应学术
必应学术中相似的文章
[Jiang, Chen]的文章
[Bedding, Timothy R.]的文章
[Stassun, Keivan G.]的文章
相关权益政策
暂无数据
收藏/分享
文件名: TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

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。