Effective Temperature Scale and Bolometric Corrections

Details Effective Temperature Scale and Bolometric Corrections Effective Temperature Scale and Bolometric Corrections

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke1891g&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 1891. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Stellar Models And Concepts

Scientific paper

The conversion from an observational quantity, such as the color index or the spectral type, to the effective temperature (Teff) of a star is known as the effective TEMPERATURE SCALE. Bolometric corrections are required in the calculation of the luminosity of a star if the flux from the star has not been observed over the entire ELECTROMAGNETIC SPECTRUM....

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