The HARPS search for southern extra-solar planets: XLII. A system of Earth-mass planets around the nearby M dwarf YZ Ceti

Exoplanet surveys have shown that systems with multiple low-mass planets on compact orbits are common. Except for a few cases, however, the masses of these planets are generally unknown. At the very end of the main sequence, host stars have the lowest mass and hence offer the largest reflect motion...

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Detalles Bibliográficos
Publicado:	2017
Materias:	Planetary systems Stars: individual: YZ Cet Stars: late-type Techniques: radial velocities Extrasolar planets Planets Stars Dynamical model Mean motion resonances Minimum mass Planetary system Radial velocity Stars: individual Stars:late type Orbits
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v605_n_p_AstudilloDefru http://hdl.handle.net/20.500.12110/paper_00046361_v605_n_p_AstudilloDefru
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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