Database of low-mass binaries - Development and applications

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Binary Stars, Data Bases, Stellar Mass, Dwarf Stars, Stellar Physics, Stellar Spectrophotometry, Stellar Motions, Stellar Flares, Stellar Orbits, Stellar Temperature

Scientific paper

The data base for low-mass binaries is designed to allow a user to obtain all published information about any dwarf star of spectral type M0 that is a component of a binary or a multiple system. The data base stores the following data: cross-identifications, coordinates, proper motions, distances, orbital parameters, photometric and spectroscopic data, information on flare activity, data on kinematics, age and population, and astrophysical parameters, such as absolute magnitudes, luminosities, effective temperatures, radii, and masses. Different designation systems for components of multiple stars are also discussed. As an application, the data on the dynamic masses and multicolor photometry of 53 M-type components of binary or multiple systems have been collected, and refined masses and luminosities are used to test the theoretical and empirical mass-luminosity relations for low-mass stars. (Abstract only).

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