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Cambridge University Press, Proceedings of the International Astronomical Union, S299(8), p. 277-278, 2013

DOI: 10.1017/s1743921313008570

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

Journal article published in 2013 by Jean-Loup Baudino, Bruno Bézard ORCID, Anthony Boccaletti, Mickael Bonnefoy, Anne-Marie Lagrange
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

AbstractWe present a radiative-convective equilibrium model for young giant exoplanets. Model predictions are compared with the existing photometric measurements of the planet β 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.