The BT-Settl Model Atmospheres for Stars, Brown Dwarfs and Planets

F. Allard

doi:10.1017/S1743921313008545

Abstract

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We present a grid of stellar and substellar atmosphere models covering the range from solar-mass stars to the latest-type T and Y dwarfs with a single setup. For the first time our synthetic spectra and photometry reproduce the formation of clouds and in particular their clearing at the L/T transition. The BT-Settl models also naturally explain the dustier infrared properties of planets as an effect of low surface gravity.

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The BT-Settl Model Atmospheres for Stars, Brown Dwarfs and Planets

Abstract

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References

This article has been cited by the following publications. This list is generated based on data provided by Crossref.

Article contents

The BT-Settl Model Atmospheres for Stars, Brown Dwarfs and Planets

Abstract

Keywords

References

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