The masses of the main-sequence stars

Details The masses of the main-sequence stars The masses of the main-sequence stars

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983s%26w....22..479s&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 22, Oct. 1983, p. 479-481. In German.

Computer Science

Main Sequence Stars, Stellar Mass, Eclipsing Binary Stars, Hertzsprung-Russell Diagram, Stellar Luminosity, Stellar Magnitude

Scientific paper

The methods used to calculate the masses of nearby visual double stars and of the components of eclipsing binaries are discussed, taking the accuracy of the orbital measurements and distance estimates into account. The spectral type, absolute magnitude, luminosity, and mass are listed for a number of stars, in tables based on the survey of Popper (1980). The empirical mass-luminosity relationship is illustrated with a Hertzsprung-Russell diagram.

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