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
Autores principales: Bonfils, X., Astudillo-Defru, N., Díaz, R., Almenara, J.-M., Forveille, T., Bouchy, F., Delfosse, X., Lovis, C., Mayor, M., Murgas, F., Pepe, F., Santos, N.C., Ségransan, D., Udry, S., Wünsche, A.
Formato: JOUR
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: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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