The mass-luminosity relationship for solar-type stars

Details The mass-luminosity relationship for solar-type stars The mass-luminosity relationship for solar-type stars

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..649v&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 649-651 (SEE N89-25819 19-92)

Physics

Double Stars, Stellar Luminosity, Stellar Mass, Stellar Physics, Sun, Calibrating, Optical Properties, Stellar Parallax

Scientific paper

The mass-luminosity relationship for solar-type stars was reinvestigated using data from the Yale Parallax Catalog and published orbits and mass ratios for the relevant visual double stars. The results confirm that to within the errors of the data, the Sun lies essentially on the mean relationship for the nearby stars. If there is to be further progress in the definition of the mass-luminosity relationship, then the accuracy of the trigonometric parallaxes must be improved substantially.

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