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- W2160335211 abstract "▪ Abstract As progressively cooler stellar and substellar objects are discovered, the presence first of molecules and then of condensed particulates greatly complicates the understanding of their physical properties. Accurate model atmospheres that include these processes are the key to establishing their atmospheric parameters. They play a crucial role in determining structural characteristics by setting the surface conditions of model interiors and providing transformations to the various observational planes. They can reveal the spectroscopic properties of brown dwarfs and help establish their detectability. In this paper, we review the current state-of-the-art theory and modeling of the atmospheres of very low mass stars, including the coolest known M dwarfs, M subdwarfs, and brown dwarfs, i.e. T eff ≤ 4,000 K and −4.0 ≤ [M/H] ≤ +0.0. We discuss ongoing efforts to incorporate molecular and grain opacities in cool stellar spectra, as well as the latest progress in (a) deriving the effective temperature scale of M dwarfs, (b) reproducing the lower main sequences of metal-poor subdwarfs in the halo and globular clusters, and (c) results of the models related to the search for brown dwarfs." @default.
- W2160335211 created "2016-06-24" @default.
- W2160335211 creator A5018147165 @default.
- W2160335211 creator A5019593013 @default.
- W2160335211 creator A5027068088 @default.
- W2160335211 creator A5057058925 @default.
- W2160335211 date "1997-09-01" @default.
- W2160335211 modified "2023-09-28" @default.
- W2160335211 title "MODEL ATMOSPHERES OF VERY LOW MASS STARS AND BROWN DWARFS" @default.
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