No CrossRef data available.
Article contents
Nonlinear Convective Pulsation Models of Second Overtone SMC Cepheids
Published online by Cambridge University Press: 12 April 2016
Abstract
Nonlinear convective pulsation models representative of SMC Cepheids pulsating in the second overtone mode are presented. Model predictions are compared with observations and implications are derived for second overtone selection criteria. The role of overtone Cepheids as distance indicators is finally investigated and the derived distance scale is at odds with the so called short distance scale.
- Type
- Part 3. Nonlinear Effects in Pulsating Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002