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Effective Temperatures and Angular Diameters of A–G Main Sequence Stars

Published online by Cambridge University Press:  12 April 2016

I.N. Glushneva ,
I.B. Voloshina  and
L.N. Knyazeva
I.N. Glushneva
Affiliation:
Sternberg Astronomical Institute, Moscow 119899, Russia
I.B. Voloshina
Affiliation:
Sternberg Astronomical Institute, Moscow 119899, Russia
L.N. Knyazeva
Affiliation:
Fessenkov Astrophysical Institute, Alma-Ata 480068, Kazakhstan

Abstract

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For 9 stars of A5–G2 spectral type interval IV and V luminosity classes effective temperatures, bolometric corrections, radii, angular diameters and luminosities were obtained by means of the infrared flux method in the modification by Blackwell et al. (1980).

Type
II. Atmospheres, a window to the interior
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 153 - 155
Copyright
Copyright © Astronomical Society of the Pacific 1993

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