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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

References

Blackwell, D.E., Shallis, M.J. 1977, M.N.R.A.S., 180, 177 Google Scholar
Blackwell, D.E., Petford, A.D., Shallis, M.J. 1980, Astr.Ap., 82, 249.Google Scholar
Code, A.D. and Meade, M.R. 1979, Ap. J. Supplements, 39, 195.CrossRefGoogle Scholar
Dreiling, L.A., Bell, R.A. 1980, Ap.J., 241, 736.Google Scholar
Glushneva, I.N., Kharitonov, A.V., Knyazeva, L.N., Shenavrin, V.I. 1992, Astr.Ap.Suppl., 92, 1.Google Scholar
Hayes, D.S. 1985, Calibration of Fundamental Stellar Quantities, in IAU Symposium 111, ed. Hayes, D.S., Pasinetti, L.E. and Davis Philip, A.G., p. 247.Google Scholar
Heck, A., Egret, D., Jaschek, M., Jashek, C. 1984, IUE Low–dispersion Spectra Reference atlas. Part 1: Normal Stars. ESA SP-1052.Google Scholar
Johnson, H.L., Mitchell, R.I., Iriarte, B., Wisniewski, W.Z. 1966, Comm.Lun.Planet.Lab., 4, 99.Google Scholar
Johnson, H.L. 1966, Ann.Rev.Astr. Ap., 4, 193.Google Scholar
Johnson, H.L., Mitchell, R.I. 1975, Rev.Mex.Astr.Astrof. 1, 299.Google Scholar
Koornneef, J. 1983, Astr. Ap., 128, 84.Google Scholar
Kurucz, R.L. 1979, Ap.J.Supplements, 40, 1.Google Scholar
Selby, M.J., Hepburn, I., Blackwell, D.E. et al. 1988, Astr.Ap.Suppl., 74, 127.Google Scholar
Saxner, M., Hammarback, G. 1985, Astr. Ap., 151, 372.Google Scholar
Straizys, V., Kuriliene, G. 1981, Astrophys. and Space Sci., 80, 353.Google Scholar
Wu, C.C., Crenshaw, D.M., Blackwell, J.H., et al. 1991, The IAU Ultraviolet Spectral Atlas, Addendum 1, International Ultraviolet Explorer (IUE) NASA NewsletterGoogle Scholar