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

Earth and Planetary Astrophysics 2014-01-20 v1
Authors: 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.

Keywords

radiative-convective equilibrium young giant exoplanets beta Pictoris b photometric measurements spectroscopic observations SPHERE

Cite

@article{arxiv.1401.4272,
  title  = {A radiative-convective equilibrium model for young giant exoplanets: Application to beta Pictoris b},
  author = {Jean-Loup Baudino and Bruno Bézard and Anthony Boccaletti and Mickael Bonnefoy and Anne-Marie Lagrange},
  journal= {arXiv preprint arXiv:1401.4272},
  year   = {2014}
}

Comments

2 pages, 1 figure, Proceedings IAUS 299

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