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- W2093765135 abstract "The angular diameters and surface gravities derived for pulsating and non-pulsating yellow supergiants from comparison of observed and computed UVBGRI photometry are generally consistent with previous absolute magnitude and radius values as well as evolutionary calculations without mass loss; together they yield refined estimates of the basic physical properties of these stars. Fernie's hypothesis of overtone pulsation for several Cepheids is more consistent than fundamental pulsation is with our data for these stars. Values of the pulsation constant Q show a gradual increase with increasing period. Good correlations of radius with period and surface brightness with (B–V)0 yield a period–luminosity–colour relationship." @default.
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- W2093765135 date "1971-04-01" @default.
- W2093765135 modified "2023-09-26" @default.
- W2093765135 title "Radii, Luminosities, and Masses from Six-Colour Fitting of Galactic Cepheids and other Supergiants" @default.
- W2093765135 doi "https://doi.org/10.1093/mnras/152.1.133" @default.
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