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- W3034447800 abstract "M dwarfs are discussed as targets for planet detection as these stars are less massive, less luminous and have smaller radii, making it possible to detect smaller and lighter planets. Therefore M-dwarfs could prove to be a valuable source for examining the lower mass end of planet distribution, In order to do that, the characteristics of the host stars must be well studied. We study the ATLAS9, MARCS and D-P stellar atmosphere model families in the M-dwarf parameter space. We examine the differences in the (Tgas, pgas) structures, synthetic photometric fluxes and related colour indices. We find discrepancies in the hotter regions of the stellar atmosphere between the ATLAS and MARCS models. The MARCS and D-P models agree to a better extend with variances of less than 300 K. We compile and compare the broad-band synthetic photometric fluxes of all models for the Johnson UBVRI and 2MASS JHKs filter systems." @default.
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- W3034447800 date "2013-07-01" @default.
- W3034447800 modified "2023-09-24" @default.
- W3034447800 title "The impact of M-dwarf atmosphere modelling on planet detection" @default.
- W3034447800 hasPublicationYear "2013" @default.
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