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Stellar rotation
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ISBN: 1107119588 0511009631 1280421266 9786610421268 0511172540 0511151365 0511302061 0511546041 0511049692 9780511009631 0511034458 9780511034459 9780521772181 0521772184 9780511546044 0521772184 9780521037693 0521037697 Year: 2000 Volume: 36 Publisher: Cambridge New York Cambridge University Press

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Abstract

Like the Earth and planets, stars rotate. Understanding how stars rotate is central to modelling their structure, formation and evolution, and how they interact with their environment and companion stars. This authoritative volume, first published in 2000, provides a lucid introduction to stellar rotation and the definitive reference to the subject. It combines theory and observation in a comprehensive survey of how the rotation of stars affects the structure and evolution of the Sun, single stars and close binaries. This book will be of primary interest to graduate students and researchers studying solar and stellar rotation and close binary systems. It will also appeal to those with a more general interest in solar and stellar physics, star formation, binary stars and the hydrodynamics of rotating fluids - including geophysicists, planetary scientists and plasma physicists.

Differential rotation and stellar convection : sun and solar-type stars
Author:
ISBN: 2881240666 2881243266 Year: 1989 Publisher: New York : Gordon and Breach Science Publishers,

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Part One is a history of the pioneers in the field of stellar rotation : the attempted solutions, and the small and large steps forward that comprise the backdrop from which the book proceeds. The various sources of differential rotation are discussed in Part Two, the book's main section, which deals with the turbulent transport of energy and angular momentum. In Part three, the previously used formulations are verified with a simple linearized turbulence theory, and the turbulence model best describing the solar convection zone is discussed. Through formulae and analyses, Differential Rotation and Stellar Convection effectively analyzes the reasons why the sun rotates as it does.


Book
Rotating Relativistic Stars.
Authors: ---
ISBN: 9780511977596 9780521872546 9781107308367 1107308364 9781107313910 1107313910 051197759X 9781107306165 1107306167 0521872545 1107301084 9781107301085 1107233623 9781107233621 1107305411 9781107305410 1299399045 9781299399044 1107311713 9781107311718 Year: 2013 Publisher: Cambridge Cambridge University Press

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Abstract

The masses of neutron stars are limited by an instability to gravitational collapse and an instability driven by gravitational waves limits their spin. Their oscillations are relevant to x-ray observations of accreting binaries and to gravitational wave observations of neutron stars formed during the coalescence of double neutron-star systems. This volume includes more than forty years of research to provide graduate students and researchers in astrophysics, gravitational physics and astronomy with the first self-contained treatment of the structure, stability and oscillations of rotating neutron stars. This monograph treats the equations of stellar equilibrium; key approximations, including slow rotation and perturbations of spherical and rotating stars; stability theory and its applications, from convective stability to the r-mode instability; and numerical methods for computing equilibrium configurations and the nonlinear evolution of their oscillations. The presentation of fundamental equations, results and applications is accessible to readers who do not need the detailed derivations.


Book
Studying stellar rotation and convection : theoretical background and seismic diagnostics
Author:
ISBN: 3642333796 364233380X Year: 2013 Publisher: Berlin ; New York : Springer,

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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.


Book
Physics, formation and evolution of rotating stars
Authors: ---
ISBN: 354076948X 9786611955151 1281955159 3540769498 Year: 2009 Publisher: Berlin ; Heidelberg : Springer-Verlag,

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Rotation is ubiquitous at each step of stellar evolution, from star formation to the final stages, and it affects the course of evolution, the timescales and nucleosynthesis. Stellar rotation is also an essential prerequisite for the occurrence of Gamma-Ray Bursts. In this book the author thoroughly examines the basic mechanical and thermal effects of rotation, their influence on mass loss by stellar winds, the effects of differential rotation and its associated instabilities, the relation with magnetic fields and the evolution of the internal and surface rotation. Further, he discusses the numerous observational signatures of rotational effects obtained from spectroscopy and interferometric observations, as well as from chemical abundance determinations, helioseismology and asteroseismology, etc. On an introductory level, this book presents in a didactical way the basic concepts of stellar structure and evolution in "track 1" chapters. The other more specialized chapters form an advanced course on the graduate level and will further serve as a valuable reference work for professional astrophysicists.

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