A temperate exo-Earth around a quiet M dwarf at 3.4 parsec

The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of the atmosphere of Earth-size worlds. The forthcoming generation of extremely large telescopes (ELTs)...

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Detalles Bibliográficos
Publicado:	2018
Materias:	Planetary systems stars: late-Type techniques: radial velocities Earth atmosphere Photometry Planets Solar radiation Stars Surveys Angular separation Extremely Large Telescopes High contrast imaging Magnetic activity Planetary system Radial-velocity observations Stars:late type Techniques: radial velocities Orbits
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v613_n_p_Bonfils http://hdl.handle.net/20.500.12110/paper_00046361_v613_n_p_Bonfils
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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