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Consequences of Rotational Mixing in late Type Massive Stars
Published online by Cambridge University Press: 04 August 2017
Extract
We have examined further the consequences of mixing induced by rotation in massive stars (Pop I composition: X = 0.7; Y = 0.27) in the mass range 40–100 M⊙. The basic physics and a detailed examination for a 60 M⊙ model has recently been published (Sreenivasan and Wilson 1985b), as has a detailed examination of supergiants without such mixing (Sreenivasan and Wilson 1985a). We shall therefore not go into the background of our computation here, but merely summarize our present findings.
- Type
- Poster Papers 3
- Information
- Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 385 - 387
- Copyright
- Copyright © Reidel 1986