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Three-Dimensional Representation of A0–G5 Stars

Published online by Cambridge University Press:  07 February 2017

B. Hauck
B. Hauck*
Affiliation:
Institut d'Astronomie de l'Université de Lausanne et Observatoire de Genève, Suisse

Abstract

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It is possible to obtain for the stars of the spectral type included between A0 and G5 three parameters respectively correlated with the effective temperature, the luminosity and the blanketing. A method to determine the absolute magnitude is given.

Résumé

Résumé

Il est possible d'obtenir pour les étoiles de type spectral compris entre A0 et G5 trois paramètres corrélés respectivement avec la température effective, la luminosité et le blanketing. Une méthode de détermination de la magnitude absolue est donnée.

Type
Part IV: Absolute Magnitude Determinations from Hydrogen-Line Photometry
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 117 - 119
Copyright
Copyright © Reidel 1973 

References

Références

Gliese, W.: 1969, Veröffentl. Astron. Rechen-Inst. Heidelberg , No. 22.Google Scholar
Goy, G.: 1971, Publ. Obs. Genève , No. 78.Google Scholar
Hauck, B.: 1968, Publ. Obs. Genève , No. 75.Google Scholar
Heckmann, O. et Johnson, H. L.: 1956, Astrophys. J. 124, 477.Google Scholar
Johnson, H. L. et Knuckles, C. F.: 1955, Astrophys. J. 122, 209.Google Scholar
Oke, J. B.: 1957, Astrophys. J. 126, 509.Google Scholar
Oke, J. B.: 1959, Astrophys. J. 130, 487.CrossRefGoogle Scholar
Oke, J. B. et Conti, P. S.: 1966, Astrophys. J. 143, 134.Google Scholar
Roman, N.: 1952, Astrophys. J. 116, 122.Google Scholar
Rufener, F.: 1971, Astron. Astrophys. Suppl. Ser. 4, 43.Google Scholar
Strömgren, B.: 1963, Stars and Stellar Systems 3, 123.Google Scholar