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The critical mass for the overstability of massive zero-age main sequence stars
Published online by Cambridge University Press: 03 August 2017
Abstract
The linear stability of massive extreme Pop I stars at the main sequence is investigated with a full nonadiabatic treatment. Contrary to earlier beliefs these stars become vibrationally unstable only beyond a critical mass as high as 440 M⊙ at the main sequence.
- Type
- Chapter 6: Excitation and Damping of Solar and Stellar Oscillations
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 399 - 402
- Copyright
- Copyright © Reidel 1988