Arid
DOI10.1051/0004-6361/201834890
The SOPHIE search for northern extrasolar planets XV. A warm Neptune around the M dwarf Gl 378
Hobson, M. J.1; Delfosse, X.2; Astudillo-Defru, N.3; Boisse, I1; Diaz, R. F.4,5; Bouchy, F.6; Bonfils, X.2; Forveille, T.2; Arnold, L.7; Borgniet, S.2; Bourrier, V6; Brugger, B.1; Salazar, N. Cabrera2; Courcol, B.1; Dalal, S.8; Deleuil, M.1; Demangeon, O.9; Dumusque, X.6; Hara, N.6,11; Hebrard, G.7,8; Kiefer, F.8; Lopez, T.1; Mignon, L.2; Montagnier, G.7,8; Mousis, O.1; Moutou, C.1,12; Pepe, F.6; Rey, J.6; Santerne, A.1; Santos, N. C.9,10; Stalport, M.6; Segransan, D.6; Udry, S.6; Wilson, P. A.8,13,14
通讯作者Hobson, M. J.
来源期刊ASTRONOMY & ASTROPHYSICS
ISSN0004-6361
EISSN1432-0746
出版年2019
卷号625
英文摘要We present the detection of a warm Neptune orbiting the M dwarf Gl 378, using radial velocity measurements obtained with the SOPHIE spectrograph at the Observatoire de Haute-Provence. The star was observed in the context of the SOPHIE exoplanet consortium's sub-programme dedicated to finding planets around M dwarfs. Gl 378 is an M1 star, of solar metallicity, at a distance of 14.96 pc. The single planet detected, Gl 378 b, has a minimum mass of 13.02 M-Earth and an orbital period of 3.82 days, which place it at the lower boundary of the hot Neptune desert. As one of only a few such planets around M dwarfs, Gl 378 b provides important clues to the evolutionary history of these close-in planets. In particular, the eccentricity of 0.1 may point to a high-eccentricity migration. The planet may also have lost part of its envelope due to irradiation.
英文关键词techniques: radial velocities planetary systems stars: late-type stars: individual: Gl 378
类型Article
语种英语
国家France ; Chile ; Argentina ; Switzerland ; Portugal ; USA ; England
开放获取类型Green Submitted, hybrid
收录类别SCI-E
WOS记录号WOS:000466318100003
WOS关键词MASS ; ROTATION ; TRANSIT ; STARS
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
资源类型期刊论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/214427
作者单位1.Aix Marseille Univ, LAM, CNES, CNRS, Marseille, France;
2.Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France;
3.Univ Concepcion, Dept Astron, Casilla 160-C, Concepcion, Chile;
4.Univ Buenos Aires, Fac Ciencias Exactas & Nat, Buenos Aires, DF, Argentina;
5.Univ Buenos Aires, CONICET, IAFE, Buenos Aires, DF, Argentina;
6.Univ Geneva, Observ Astron, 51 Chemin Maillettes, CH-1290 Versoix, Switzerland;
7.Aix Marseille Univ, CNRS, Observ Haute Provence, Inst Pytheas UMS 3470, F-04870 St Michel Lobservatoi, France;
8.Univ Paris 06, UMR7095 CNRS, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France;
9.Univ Porto, CAUP, Inst Astrofis & Ciencias Esp, Rua Estrelas, P-4150762 Porto, Portugal;
10.Univ Porto, Fac Ciencias, Dept Fis & Astron, Rua Campo Alegre, P-4169007 Porto, Portugal;
11.UPMC, PSL, Observ Paris, CNRS UMR8028,ASD IMCCE, 77 Ave Denfert Rochereau, F-75014 Paris, France;
12.Canada France Hawaii Telescope Corp, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743 USA;
13.Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England;
14.Univ Warwick, Ctr Exoplanets & Habitabil, Coventry CV4 7AL, W Midlands, England
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GB/T 7714
Hobson, M. J.,Delfosse, X.,Astudillo-Defru, N.,et al. The SOPHIE search for northern extrasolar planets XV. A warm Neptune around the M dwarf Gl 378[J],2019,625.
APA Hobson, M. J..,Delfosse, X..,Astudillo-Defru, N..,Boisse, I.,Diaz, R. F..,...&Wilson, P. A..(2019).The SOPHIE search for northern extrasolar planets XV. A warm Neptune around the M dwarf Gl 378.ASTRONOMY & ASTROPHYSICS,625.
MLA Hobson, M. J.,et al."The SOPHIE search for northern extrasolar planets XV. A warm Neptune around the M dwarf Gl 378".ASTRONOMY & ASTROPHYSICS 625(2019).
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