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Theoretical Spectral Models of the Planet HD 209458b with a Thermal Inversion and Water Emission Bands
Adam Burrows, Ivan Hubeny, Jano Budaj +2
We find that a theoretical fit to all the HD 209458b data at secondary eclipse requires that the dayside atmosphere of HD 209458b have a thermal inversion and a stratosphere. This…
Argon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars
Thierry Lanz, Katia Cunha, Jon Holtzman +1
Argon abundances have been derived for a sample of B main-sequence stars in the Orion association. The abundance calculations are based on NLTE metal line-blanketed model atmospher…
A Mass Function Constraint on Extrasolar Giant Planet Evaporation Rates
W. B Hubbard, M. Hattori, A. Burrows +1
The observed mass function for all known extrasolar giant planets (EGPs) varies approximately as M^{-1} for mass M between 0.2 Jupiter masses (M_J) and 5 M_J. In order to study eva…