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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
DOI10.3847/1538-3881/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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