Artículo
The SOPHIE search for northern extrasolar planets XV: A warm Neptune around the M dwarf Gl 378
Hobson, M. J.; Delfosse, X.; Astudillo Defru, N.; Boisse, I.; Diaz, Rodrigo Fernando
; Bouchy, F.; Bonfils, X.; Forveille, T.; Arnold, L.; Borgniet, S.; Bourrier, V.; Brugger, B.; Cabrera Salazar, N.; Courcol, B.; Dalal, S.; Deleuil, M.; Demangeon, O.; Dumusque, X.; Hara, N.; Hébrard, G.; Kiefer, F.; Lopez, T.; Mignon, L.; Montagnier, G.; Mousis, O.; Moutou, C.; Pepe, F.; Rey, J.; Santerne, A.; Santos, N. C.; Stalport, M.; Ségransan, D.; Udry, S.; Wilson, P. A.

Fecha de publicación:
05/2019
Editorial:
EDP Sciences
Revista:
Astronomy and Astrophysics
ISSN:
0004-6361
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
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 MEarth 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.
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Articulos(IAFE)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Citación
Hobson, M. J.; Delfosse, X.; Astudillo Defru, N.; Boisse, I.; Diaz, Rodrigo Fernando; et al.; The SOPHIE search for northern extrasolar planets XV: A warm Neptune around the M dwarf Gl 378; EDP Sciences; Astronomy and Astrophysics; 625; 5-2019; 1-10
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