The surface-brightness method and the dependence of bolometric correction on stellar effective temperature

Details The surface-brightness method and the dependence of bolometric correction on stellar effective temperature The surface-brightness method and the dependence of bolometric correction on stellar effective temperature

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...64g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Jan.-Feb. 1991, p. 64-71. In Russian.

Physics

3

Bolometers, Brightness Temperature, Stellar Luminosity, Stellar Temperature, Color-Color Diagram, Stellar Spectra

Scientific paper

Relationships between the surface-brightness parameter and dereddened
color indices (B-V)0 and (V-R)0, as well as between the bolometric
correction and the effective temperature, are constructed using data on
the physical characteristics of 228 stars with Teff greater than 4700 K.
Simple analytical expressions are obtained for these relationships.

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