The mass-spectrum relation for main-sequence stars

Details The mass-spectrum relation for main-sequence stars The mass-spectrum relation for main-sequence stars

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..143s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 143-151) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 8

Astronomy and Astrophysics

Astronomy

8

Eclipsing Binary Stars, Main Sequence Stars, Mass Ratios, Stellar Mass, Root-Mean-Square Errors, Stellar Spectra

Scientific paper

From 240 main-sequence stars with well-determined masses a new mass-spectrum relation is obtained, which differs appreciably in certain intervals of spectral types from the mass-spectrum relations of Allen and Trimble. The accuracy of mass determination for the components of eclipsing binary systems of different types from their spectra given in the General Catalogue of Variable Stars (3rd edition) and in its supplements is evaluated.

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