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Radiative equilibrium models of “hot Jupiters”
Published online by Cambridge University Press: 26 May 2016
Abstract
We present an extension of our equilibrium model, initially applied to 51 Peg b (Goukenleuque et al. 2000), to other irradiated extrasolar planets with different orbital distances (up to 1 AU). The model yields the mean atmospheric thermal structure and predicts the reflected spectral flux as well as the thermal flux emerging from such planets, in the visible and in the infrared wavelength ranges.
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- Part III: Structure and atmospheres of planets
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- Copyright © Astronomical Society of the Pacific 2004