HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS
文献类型:期刊论文
作者 | Wang,Songhu1; Jones,Matias2; Shporer,Avi3; Fulton,Benjamin J.4,5; Paredes,Leonardo A.6; Trifonov,Trifon7; Kossakowski,Diana7; Eastman,Jason8; Redfield,Seth9; Günther,Maximilian N.3 |
刊名 | The Astronomical Journal |
出版日期 | 2019-01-14 |
卷号 | 157期号:2 |
ISSN号 | 0004-6256 |
关键词 | planetary systems planets and satellites: detection stars: individual (TIC 290131778-TOI 123-HD 202772 techniques: radial velocities |
DOI | 10.3847/1538-3881/aaf1b7 |
英文摘要 | Abstract We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V?=?8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known. |
语种 | 英语 |
出版者 | The American Astronomical Society |
WOS记录号 | IOP:0004-6256-157-2-AAF1B7 |
源URL | [http://ir.bao.ac.cn/handle/114a11/24646] |
专题 | 中国科学院国家天文台 |
作者单位 | 1.Department of Astronomy, Yale University, New Haven, CT 06511, USA; song-hu.wang@yale.edu 2.European Southern Observatory, Casilla 19001, Santiago, Chile 3.Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 4.California Institute of Technology, Pasadena, CA 91125, USA 5.IPAC-NASA Exoplanet Science Institute Pasadena, CA 91125, USA 6.Physics and Astronomy Department, Georgia State University, Atlanta, GA 30302, USA 7.Max-Planck-Institut für Astronomie, K?nigstuhl 17, D-69117 Heidelberg, Germany 8.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 9.Astronomy Department and Van Vleck Observatory, Wesleyan University, Middletown, CT 06459, USA 10.Harvard Society of Fellows, 78 Mount Auburn Street, Cambridge, MA 02138, USA |
推荐引用方式 GB/T 7714 | Wang,Songhu,Jones,Matias,Shporer,Avi,et al. HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS[J]. The Astronomical Journal,2019,157(2). |
APA | Wang,Songhu.,Jones,Matias.,Shporer,Avi.,Fulton,Benjamin J..,Paredes,Leonardo A..,...&Laughlin,Gregory.(2019).HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS.The Astronomical Journal,157(2). |
MLA | Wang,Songhu,et al."HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS".The Astronomical Journal 157.2(2019). |
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来源:国家天文台
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