The SOPHIE search for northern extrasolar planets XV. A Warm Neptune around the M-dwarf Gl378. (arXiv:1902.05998v1 [astro-ph.EP])
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We present the detection of a Warm Neptune orbiting the M-dwarf Gl378, 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 exoplanets consortium’s subprogramme dedicated to finding planets around
M-dwarfs. Gl378 is an M1 star, of solar metallicity, at a distance of 14.96 pc.
The single planet detected, Gl378 b, has a minimum mass of 13.02 $rm
M_{Earth}$ 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, Gl378 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.

We present the detection of a Warm Neptune orbiting the M-dwarf Gl378, 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 exoplanets consortium’s subprogramme dedicated to finding planets around
M-dwarfs. Gl378 is an M1 star, of solar metallicity, at a distance of 14.96 pc.
The single planet detected, Gl378 b, has a minimum mass of 13.02 $rm
M_{Earth}$ 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, Gl378 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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