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Population I Cepheids – Theory and Observation
Published online by Cambridge University Press: 07 February 2017
Abstract
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