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Studying Stellar Rotation and Convection [electronic resource] : Theoretical Background and Seismic Diagnostics / edited by Mariejo Goupil, KȨvin Belkacem, Coralie Neiner, Francois Ligniȿres, John J. Green.

Por: Goupil, Mariejo [editor.]Colaborador(es): Belkacem, KȨvin [editor.] | Neiner, Coralie [editor.] | Ligniȿres, Francois [editor.] | Green, John J [editor.]Tipo de material: TextoTextoSeries Lecture Notes in Physics, 865Editor: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2013Descripción: XI, 261 p. 85 illus., 46 illus. in color. online resourceTipo de contenido: text Tipo de medio: computer Tipo de portador: online resourceISBN: 9783642333804Trabajos contenidos: SpringerLink (Online service)Tema(s): Physics | Physics | Astrophysics and Astroparticles | Astronomy, Observations and Techniques | Numerical and Computational PhysicsFormatos físicos adicionales: Sin títuloClasificación CDD: 523.01 Clasificación LoC:QB460-466Recursos en línea: de clik aquí para ver el libro electrónico
Contenidos:
Springer eBooksResumen: This volume synthesizes the results of work carried out by several international teams of the SIROCO (Seismology for Rotation and Convection) collaboration. It provides the theoretical background required to interpret the huge quantity of high-quality observational data recently provided by space experiments such as CoRoT and Kepler. Asteroseismology allows astrophysicists to test, to model and to understand stellar structure and evolution as never before. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book offers the reader solid theoretical background knowledge and adapted seismic diagnostic techniques.
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Rotation and Associated Seismology -- Modeling and Rotating Stars -- 2D Oscillation of Rotating Stars -- Seismology of Rotating Stars -- Convection and Associated Seismology -- Turbulent Convection in Stellar Surface Layers -- Dynamical Instabilities.

This volume synthesizes the results of work carried out by several international teams of the SIROCO (Seismology for Rotation and Convection) collaboration. It provides the theoretical background required to interpret the huge quantity of high-quality observational data recently provided by space experiments such as CoRoT and Kepler. Asteroseismology allows astrophysicists to test, to model and to understand stellar structure and evolution as never before. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book offers the reader solid theoretical background knowledge and adapted seismic diagnostic techniques.

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