Discovery of a young low-mass brown dwarf transiting a fast-rotating F-type star by the Galactic Plane eXoplanet (GPX) survey

被引:14
|
作者
Benni, P. [1 ]
Burdanov, A. Y. [2 ,3 ]
Krushinsky, V. V. [4 ]
Bonfanti, A. [5 ,6 ]
Hebrard, G. [7 ,8 ]
Almenara, J. M. [9 ]
Dalal, S. [7 ]
Demangeon, O. D. S. [10 ]
Tsantaki, M. [11 ]
Pepper, J. [12 ]
Stassun, K. G. [13 ]
Vanderburg, A. [14 ]
Belinski, A. [15 ]
Kashaev, F. [16 ]
Barkaoui, K. [17 ,18 ]
Kim, T. [19 ]
Kang, W. [19 ]
Antonyuk, K. [20 ]
Dyachenko, V. V. [21 ]
Rastegaev, D. A. [21 ]
Beskakotov, A. [21 ,22 ]
Mitrofanova, A. A. [21 ]
Pozuelos, F. J. [6 ,17 ]
Kuznetsov, E. D. [23 ]
Popov, A. [23 ]
Kiefer, F. [7 ]
Wilson, P. A. [24 ,25 ]
Ricker, G. [26 ,27 ]
Vanderspek, R. [26 ,27 ]
Latham, D. W. [28 ]
Seager, S. [2 ,26 ,27 ,29 ]
Jenkins, J. M. [30 ]
Sokov, E. [22 ,31 ]
Sokova, I [22 ,31 ]
Marchini, A. [32 ]
Papini, R. [33 ]
Salvaggio, F. [33 ]
Banfi, M. [33 ]
Basturk, O. [34 ]
Torun, S. [34 ]
Yalcinkaya, S. [34 ]
Ivanov, K. [35 ]
Valyavin, G. [20 ,21 ,22 ]
Jehin, E. [6 ]
Gillon, M. [17 ]
Pakstiene, E. [36 ]
Hentunen, V-P [37 ]
Shadick, S. [38 ]
Bretton, M. [39 ]
Wunsche, A. [39 ]
机构
[1] Acton Sky Portal Private Observ, Acton, MA 01720 USA
[2] MIT, Dept Earth Atmospher & Planetary Sci, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[3] Inst Astrofis Canarias, Via Lactea S-N, E-38205 Tenerife, Spain
[4] Ural Fed Univ, Lab Astrochem Res, Mira St 19, Ekaterinburg 620002, Russia
[5] Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria
[6] Univ Liege, Space Sci Technol & Astrophys Res STAR Inst, Allee 6 Aout 17, B-4000 Liege, Belgium
[7] Univ Paris 06, Inst Astrophys Paris, UMR7095 CNRS, 98bis Blvd Arago, F-75014 Paris, France
[8] Univ Aix Marseille, Observ Haute Provence, CNRS, F-04870 St Michell Observatoire, France
[9] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France
[10] Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Porto, Portugal
[11] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy
[12] Lehigh Univ, Dept Phys, 16 Mem Dr East, Bethlehem, PA 18015 USA
[13] Vanderbilt Univ, Dept Phys & Astron, 6301 Stevenson Ctr Ln, Nashville, TN 37235 USA
[14] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
[15] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, 13 Univ Skij Pr, Moscow 119234, Russia
[16] Moscow MV Lomonosov State Univ, Fac Phys, Leninskie Gory 1, Moscow 119991, Russia
[17] Univ Liege, Astrobiol Res Unit, Allee 6 Aout 19C, B-4000 Liege, Belgium
[18] Cadi Ayyad Univ, Oukaimeden Observ, High Energy Phys & Astrophys Lab, Marrakech 40000, Morocco
[19] Natl Youth Space Ctr, Goheung 59567, Jeollanam Do, South Korea
[20] RAS, Fed State Budget Sci Inst Crimean Astrophys Obser, Nauchny 298409, Crimea, Russia
[21] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
[22] St Petersburg State Univ, Fac Math & Mech, Univ Skij Pr 28, St Petersburg 198504, Russia
[23] Ural Fed Univ, Mira St 19, Ekaterinburg 620002, Russia
[24] Univ Warwick, Ctr Exoplanets & Habitabil, Gibbet Hill Rd, Coventry CV4 7AL, W Midlands, England
[25] Univ Warwick, Dept Phys, Gibbet Hill Rd, Coventry CV4 7AL, W Midlands, England
[26] MIT, Dept Phys, Cambridge, MA 02139 USA
[27] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[28] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
[29] MIT, Dept Aeronaut & Astronaut Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[30] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[31] Russian Acad Sci, Cent Astron Observ Pulkovo, Pulkovskoje Shosse D 65, St Petersburg 196140, Russia
[32] Univ Siena, Astron Observ DSFTA, Via Roma 56, I-53100 Siena, Italy
[33] Wild Boar Remote Observ, I-50026 San Casciano In Val Pesa, FI, Italy
[34] Ankara Univ, Fac Sci, Dept Astron & Space Sci, TR-06100 Ankara, Turkey
[35] Irkutsk State Univ, K Marx Str 1, Irkutsk 664003, Russia
[36] Vilnius Univ, Inst Theoret Phys & Astron, Sauletekio Al 3, LT-10257 Vilnius, Lithuania
[37] Taurus Hill Observ, Harkamaentie 88, FI-79480 Varkaus, Finland
[38] Univ Saskatchewan, Phys & Engn Phys Dept, Saskatoon, SK S7N 5E2, Canada
[39] Baronnies Provencales Observ, Hautes Alpes Parc Nat Reg Baronnies Provencales, E-05150, Moydans, France
[40] GJP Private Observ, Elgin, OR 97827 USA
[41] Rasteau Observ, F-84110 Rasteau, France
[42] Anunaki Observ, Manzanares El Real 28410, Spain
[43] Grand Pra Private Observ, CH-1984 Les Hauderes, Switzerland
[44] Observ Ca lOu, E-08282 St Marti Sesgueioles, Spain
[45] Observ Montcabrer, C Jaume Balmes 24, E-08348 Cabrils, Spain
[46] Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA
[47] Penn State Univ, Ctr Exoplanets & Habitable Worlds, 525 Davey Lab, University Pk, PA 16802 USA
[48] Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA
[49] Swarthmore Coll, Dept Phys & Astron, 500 Coll Ave, Swarthmore, PA 19081 USA
[50] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
基金
俄罗斯科学基金会; 美国国家航空航天局;
关键词
stars: brown dwarfs; stars: individual: GPX-1; stars: rotation; surveys: Astronomical Data bases; Galaxy: disc; EVOLUTIONARY MODELS; SEARCH; COMPANIONS; DESERT; CLUSTERS; BINARY; KEPLER; K2;
D O I
10.1093/mnras/stab1567
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We announce the discovery of GPX-1 b, a transiting brown dwarf with a mass of 19.7 +/- 1.6 M-Jup and a radius of 1.47 +/- 0.10 R-Jup, the first substellar object discovered by the Galactic Plane eXoplanet (GPX) survey. The brown dwarf transits a moderately bright (V = 12.3 mag) fast-rotating F-type star with a projected rotational velocity v sin i(*) = 40 +/- 10 km s(-1). We use the isochrone placement algorithm to characterize the host star, which has effective temperature 7000 +/- 200 K, mass 1.68 +/- 0.10 M-circle dot, radius 1.56 +/- 0.10 R-circle dot, and approximate age 0.27(-0.15)(+0.09) Gyr. GPX-1 b has an orbital period of similar to 1.75 d and a transit depth of 0.90 +/- 0.03 per cent. We describe the GPX transit detection observations, subsequent photometric and speckle-interferometric follow-up observations, and SOPHIE spectroscopic measurements, which allowed us to establish the presence of a substellar object around the host star. GPX-1 was observed at 30-min integrations by TESS in Sector 18, but the data are affected by blending with a 3.4 mag brighter star 42 arcsec away. GPX-1 b is one of about two dozen transiting brown dwarfs known to date, with a mass close to the theoretical brown dwarf/gas giant planet mass transition boundary. Since GPX-1 is a moderately bright and fast-rotating star, it can be followed-up by the means of the Doppler tomography.
引用
收藏
页码:4956 / 4967
页数:12
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