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Population I Cepheids – Theory and Observation

Published online by Cambridge University Press:  07 February 2017

R. S. Stobie
R. S. Stobie*
Affiliation:
Mount Stromlo and Siding Spring Observatory, Australian National University, Canberra, Australia

Abstract

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The quantitative discrepancies between theory and observation with regard to population I Cepheids are discussed. The discrepancies cannot be reconciled by mass loss or by changes in the luminosity or effective temperature of the variables. It is concluded that the present pulsation models both linear and non-linear are in error.

Type
Part II Pulsation and the Young Disc Population
Information
Symposium - International Astronomical Union , Volume 59: Stellar Instability and Evolution , 1974 , pp. 49 - 53
Copyright
Copyright © Reidel 1974 

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