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A radiative-convective equilibrium model for young giant exoplanets: Application to β Pictoris b
Published online by Cambridge University Press: 06 January 2014
Abstract
We 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 277 - 278
- Copyright
- Copyright © International Astronomical Union 2013
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