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Uncertainties in the Position of the β Cephei Instability Strip in the HR Diagram
Published online by Cambridge University Press: 12 April 2016
Abstract
We discuss the sensitivity of the theoretical B star instability domains to the heavy element abundance Z, the adopted metal mixture, the assumed overshooting from stellar convective cores and the choice of the opacity data.
- Type
- Part 2. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 291 - 292
- Copyright
- Copyright © Astronomical Society of the Pacific 1995