Theory Of Rotating Stars


Theory Of Rotating Stars
DOWNLOAD

Download Theory Of Rotating Stars PDF/ePub or read online books in Mobi eBooks. Click Download or Read Online button to get Theory Of Rotating Stars book now. This website allows unlimited access to, at the time of writing, more than 1.5 million titles, including hundreds of thousands of titles in various foreign languages. If the content not found or just blank you must refresh this page





Theory Of Rotating Stars


Theory Of Rotating Stars
DOWNLOAD

Author : Jean Louis Tassoul
language : en
Publisher:
Release Date : 1978-01-01

Theory Of Rotating Stars written by Jean Louis Tassoul and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1978-01-01 with categories.




Theory Of Rotating Stars Psa 1 Volume 1


Theory Of Rotating Stars Psa 1 Volume 1
DOWNLOAD

Author : Jean-Louis Tassoul
language : en
Publisher: Princeton University Press
Release Date : 2015-03-08

Theory Of Rotating Stars Psa 1 Volume 1 written by Jean-Louis Tassoul and has been published by Princeton University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2015-03-08 with Science categories.


Ever since the first observations of sunspots in the early seventeenth century, stellar rotation has been a major topic in astronomy and astrophysics. Jean-Louis Tassoul synthesizes a large number of theoretical investigations on rotating stars. Drawing upon his own research, Professor Tassoul also carefully critiques various competing ideas. In the first three chapters, the author provides a short historical sketch of stellar rotation, the main observational data on the Sun and other stars on which the subsequent theory is based, and the basic Newtonian hydrodynamics used to study rotating stars. Following a discussion of some general mechanical properties of stars in a state of permanent rotation, he reviews the main techniques for determining the structure of a rotating star and its stability with respect to infinitesimal disturbances. Since the actual distribution of angular momentum within stars is still unknown, Professor Tassoul considers various models of angular momentum as well as of meridional circulation. He devotes the rest of his study to the problems concerning various groups of stars and stages in stellar evolution. Originally published in 1979. The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.



Stellar Rotation


Stellar Rotation
DOWNLOAD

Author : Jean-Louis Tassoul
language : en
Publisher: Cambridge University Press
Release Date : 2000-04-13

Stellar Rotation written by Jean-Louis Tassoul and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2000-04-13 with Science categories.


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.



Rotating Relativistic Stars


Rotating Relativistic Stars
DOWNLOAD

Author : John L. Friedman
language : en
Publisher:
Release Date : 2013

Rotating Relativistic Stars written by John L. Friedman and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013 with Electronic books categories.


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 pulls together 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"



Rotating Relativistic Stars


Rotating Relativistic Stars
DOWNLOAD

Author : John L. Friedman
language : en
Publisher: Cambridge University Press
Release Date : 2013-02-11

Rotating Relativistic Stars written by John L. Friedman and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-02-11 with Science categories.


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.



Theory Of Rotating Stars


Theory Of Rotating Stars
DOWNLOAD

Author : Jean Louis Tassoul
language : en
Publisher:
Release Date : 1978

Theory Of Rotating Stars written by Jean Louis Tassoul and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1978 with Science categories.


Ever since the first observations of sunspots in the early seventeenth century, stellar rotation has been a major topic in astronomy and astrophysics. Jean-Louis Tassoul synthesizes a large number of theoretical investigations on rotating stars. Drawing upon his own research, Professor Tassoul also carefully critiques various competing ideas. In the first three chapters, the author provides a short historical sketch of stellar rotation, the main observational data on the Sun and other stars on which the subsequent theory is based, and the basic Newtonian hydrodynamics used to study rotating stars. Following a discussion of some general mechanical properties of stars in a state of permanent rotation, he reviews the main techniques for determining the structure of a rotating star and its stability with respect to infinitesimal disturbances. Since the actual distribution of angular momentum within stars is still unknown, Professor Tassoul considers various models of angular momentum as well as of meridional circulation. He devotes the rest of his study to the problems concerning various groups of stars and stages in stellar evolution. Originally published in 1979. The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.



Physics Formation And Evolution Of Rotating Stars


Physics Formation And Evolution Of Rotating Stars
DOWNLOAD

Author : Andre Maeder
language : en
Publisher: Springer Science & Business Media
Release Date : 2008-12-19

Physics Formation And Evolution Of Rotating Stars written by Andre Maeder and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2008-12-19 with Science categories.


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.



Differential Rotation And Stellar Convection


Differential Rotation And Stellar Convection
DOWNLOAD

Author : Günther Rüdiger
language : en
Publisher: Taylor & Francis
Release Date : 1989

Differential Rotation And Stellar Convection written by Günther Rüdiger and has been published by Taylor & Francis this book supported file pdf, txt, epub, kindle and other format this book has been release on 1989 with Architecture categories.


First Published in 1989. Routledge is an imprint of Taylor & Francis, an informa company.



Neutron Stars Theory And Observation


Neutron Stars Theory And Observation
DOWNLOAD

Author : J.E Ventura
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06

Neutron Stars Theory And Observation written by J.E Ventura and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.


Some twenty-three years after the discovery of pulsars and their identification as rotating neutron stars, neutron star physics may be regarded as comingofage. Pul sars and accreting neutron stars have now been studied at every wavelength, from the initial radio observations, through optical, X-, and "{-ray, up to the very recent observations in the TeV region, while theorists have studied in some detail relevant physical processes both outside and inside neutron stars. As a result, comparisonof theory with observation provides a test ofour theoretical ideas in fields as diverse as neutron and nuclear matter, superfluidity and superconductivity, the acceleration of high energy particles, and the generation and maintenance of intense magnetic fields. For example, through observations of glitches and post glitch behavior of pulsars, it has become possible to establish the presence ofsuperfluid neutron mat ter in the inner crust of neutron stars, and to determine some of its properties, while neutron stars in compact binary systems offer one ofthe most efficient energy generation mechanisms known. It is in fact the interactive interpretation of these ,diverse pieces of information that can lead to major advances in our understanding of the physics of these exotic objects, and justifies the characterization of neutron stars as hadron physics laboratories.



Rapidly Rotating Neutron Stars In General Relativity


Rapidly Rotating Neutron Stars In General Relativity
DOWNLOAD

Author : Gregory B. Cook
language : en
Publisher:
Release Date : 1993

Rapidly Rotating Neutron Stars In General Relativity written by Gregory B. Cook and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1993 with Neutron stars categories.