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A radiative-convective equilibrium model for young giant exoplanets: Application to beta Pictoris b
Published 17 Jan 2014 in astro-ph.EP | (1401.4272v1)
Abstract: We present a radiative-convective equilibrium model for young giant exoplanets. Model predictions are compared with the existing photometric measurements of planet beta Pictoris b in the J, H, Ks, L', NB 4.05, M' bands . This model will be used to interpret future photometric and spectroscopic observations of exoplanets with SPHERE, mounted at the VLT with a first light expected mid-2014.
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