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arXiv · 1401.4272

A radiative-convective equilibrium model for young giant exoplanets: Application to beta Pictoris b

Jean-Loup Baudino·Bruno Bézard·Anthony Boccaletti·Mickael Bonnefoy·Anne-Marie Lagrange
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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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Jean-Loup Baudino, Bruno Bézard, Anthony Boccaletti, Mickael Bonnefoy, Anne-Marie Lagrange. 2014-01-17. A radiative-convective equilibrium model for young giant exoplanets: Application to beta Pictoris b. https://doi.org/10.1017/s1743921313008570

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