Carbon monoxide and water vapor in the atmosphere of the non-transiting exoplanet HD 179949 b

Context. In recent years, ground-based high-resolution spectroscopy has become a powerful tool for investigating exoplanet atmospheres. It allows the robust identification of molecular species, and it can be applied to both transiting and non-transiting planets. Radial-velocity measurements of the s...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2014-05, Vol.565, p.np-np
Hauptverfasser:	Brogi, M., de Kok, R. J., Birkby, J. L., Schwarz, H., Snellen, I. A. G.
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheres Extrasolar planets methods: data analysis Orbital velocity Planets planets and satellites: atmospheres planets and satellites: fundamental parameters Spectra Spectroscopy Stars techniques: spectroscopic Water vapor
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