Published in

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

DOI: 10.1017/s1743921313008570

Links

Tools

Export citation

Search in Google Scholar

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 was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Green circle
Postprint: archiving allowed
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

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.

Beta version