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Radii and Fluxes of Long-Period Cepheids

Published online by Cambridge University Press:  07 February 2017

A. Opolski
A. Opolski*
Affiliation:
Wroclaw Astronomical Observatory, Wroclaw, Poland

Abstract

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The radii of 9 long-period Cepheids have been determined by means of the modificated Wesselink method and some general conclusions have been formulated. The relations R – P and Fv – Mv for stars recognized as fundamental and first overtone pulsators have been established.

Type
Part V: Ground Based and Extraterrestrial Observations of Stellar Flux
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 165 - 170
Copyright
Copyright © Reidel 1973 

References

Fernie, J. D.: 1968, Astrophys. J. 151, 197.CrossRefGoogle Scholar
Fernie, J. D. and Hube, J. O.: 1967, Publ. Astron. Soc. Pacific 79, 95.CrossRefGoogle Scholar
Fernie, J. D. and Hube, J. O.: 1968, Astron. J. 73, 492.CrossRefGoogle Scholar
Latyshev, I. N.: 1964, Astron. Zh. 41, 644.Google Scholar
Opolski, A. and Krawiecka, J.: 1965, Contr. Wroclaw Astron. Obs. No. 11.Google Scholar
Parsons, S. B. and Bouw, G. D.: 1971, Monthly Notices Roy. Astron. Soc. 152, 133.CrossRefGoogle Scholar