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Theoretical Pulsations of Luminous Blue Variables
Published online by Cambridge University Press: 12 April 2016
Abstract
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Both radial and low degree and order g-mode nonradial pulsations are predicted for luminous blue variables that occur in the blue supergiant region of the Hertzsprung-Russell diagram. It is found that the radial strange modes have very large growth rates due to helium ionization in models at surface effective temperatures between 10,000 and 20,000 K.
- Type
- Part 1. The Scientific Programme
- Information
- International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 192 - 193
- Copyright
- Copyright © Astronomical Society of the Pacific 1995