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• W3100462751 startingPage "42" @default.
• W3100462751 abstract "We examine the agreement between the observed and theoretical low-mass (< 0.8 solar masses) stellar main sequence mass-radius relationship by comparing detached eclipsing binary (DEB) data with a new, large grid of stellar evolution models. The new grid allows for a realistic variation in the age and metallicity of the DEB population, characteristic of the local galactic neighborhood. Overall, our models do a reasonable job of reproducing the observational data. A large majority of the models match the observed stellar radii to within 4%, with a mean absolute error of 2.3%. These results represent a factor of two improvement compared to previous examinations of the low-mass mass-radius relationship. The improved agreement between models and observations brings the radius deviations within the limits imposed by potential starspot-related uncertainties for 92% of the stars in our DEB sample." @default.
• W3100462751 created "2020-11-23" @default.
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• W3100462751 date "2012-09-04" @default.
• W3100462751 modified "2023-09-30" @default.
• W3100462751 title "REEVALUATING THE MASS-RADIUS RELATION FOR LOW-MASS, MAIN-SEQUENCE STARS" @default.
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• W3100462751 doi "https://doi.org/10.1088/0004-637x/757/1/42" @default.
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