Rotation and mixing in stellar interiors : proceedings of the Workshop Frontiers in Stellar Structure Theory held in honor of Professor Evry Schatzman in Les Houches, France, June 19-25, 1989
The 14 papers in this collection discuss recent progress in areas such as mixing in stellar interiors, redistribution and loss of angular momentum, emphasizing in particular the effects of turbulence. An introductory review by E. Schatzman, to whom this volume is dedicated, is followed by three sect...
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| その他の著者: | , |
| フォーマット: | Livre numérique |
| 言語: | Anglais |
| 出版事項: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| シリーズ: | Lecture notes in physics
366 |
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| オンライン･アクセス: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
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Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Rotation and mixing in stellar interiors, proceedings of the Workshop Frontiers in Stellar Structure Theory held in honor of Professor Evry Schatzman in Les Houches, France, June 19-25, 1989, Berlin, Springer-Verlag, 1990, 1 vol. (XIII-182 p.), Lecture notes in physics, 3-540-53059-2 • Rotation and Mixing in Stellar Interiors, Texte imprimé, 9783662137758 • Rotation and Mixing in Stellar Interiors, Texte imprimé, 9783662137765 |
目次:
- Rotation, lithium and mixing
- Surface abundances
- Stellar rotation prior to the main sequence
- The internal rotation of the sun
- Loss of mass and angular momentum: The observational point of view
- Pre-main sequence evolutionary tracks and lithium burning
- Mass transport and mixing by waves
- Turbulent transport in stratified and rotating fluids
- Penetration and overshooting from a convection zone
- Turbulent transport in stellar radiation zones: Causes and effects
- Will a magnetic field inhibit turbulent transport?
- Fast dynamo action-A critical problem for solar magnetism
- Observational constraints on the turbulent diffusion coefficient in late type stars
- Probing stellar interiors
- Conclusion.