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Studying Stellar Rotation and Convection

Theoretical Background and Seismic Diagnostics

  • Book
  • © 2013

Overview

  • Provides the fundamentals of astroseismology with a focus on waves caused by stellar rotation and by stellar convection.
  • Gives the necessary theoretical background to interpret observations by space experiments such as CoRoT and Kepler
  • Synthesizes the results of work carried out by a collaboration of several international teams
  • Includes supplementary material: sn.pub/extras

Part of the book series: Lecture Notes in Physics (LNP, volume 865)

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Table of contents (12 chapters)

  1. Rotation and Associated Seismology

  2. Rotation and associated seismology

  3. Convection and Associated Seismology

  4. Convection and associated seismology

Keywords

About this book

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.

Editors and Affiliations

  • LESIA, Observatoire de Paris-Meudon, Meudon Cedex, France

    Mariejo Goupil, Kévin Belkacem, Coralie Neiner

  • Institut de Recherche en Astrophysique, et Planétologie, Observatoire Midi-Pyrénées, Toulouse, France

    Francois Lignières

  • Observatoire de Paris-Meudon, LESIA, Meudon, France

    John J. Green

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