Stellar Rotation

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Publisher : Cambridge University Press
ISBN 13 : 1139428322
Total Pages : 274 pages
Book Rating : 4.1/5 (394 download)

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Book Synopsis Stellar Rotation by : Jean-Louis Tassoul

Download or read book Stellar Rotation written by Jean-Louis Tassoul and published by Cambridge University Press. This book was released on 2000-04-13 with total page 274 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Stellar Rotation

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Author :
Publisher : Springer Nature
ISBN 13 : 9819733650
Total Pages : 205 pages
Book Rating : 4.8/5 (197 download)

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Book Synopsis Stellar Rotation by : Arnold Hanslmeier

Download or read book Stellar Rotation written by Arnold Hanslmeier and published by Springer Nature. This book was released on with total page 205 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Stellar Rotation

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Author :
Publisher : Springer Science & Business Media
ISBN 13 : 9401032998
Total Pages : 363 pages
Book Rating : 4.4/5 (1 download)

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Book Synopsis Stellar Rotation by : A. Slettebak

Download or read book Stellar Rotation written by A. Slettebak and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 363 pages. Available in PDF, EPUB and Kindle. Book excerpt: The International Astronomical Union Colloquium on Stellar Rotation was held at the Ohio State University in Columbus, Ohio, U.S.A. from September 8th through 11 th, 1969. Forty-four scientists from Argentina, Belgium, Canada, England, Finland, East and West Germany, Italy, Israel, Japan, The Netherlands, and the United States attended and participated in the Colloquium. The present volume, which parallels the actual program closely, contains the papers presented at the Colloquium plus most of the discussion following those papers. The Colloquium was sponsored by the International Astronomical Union, the Ohio State University, and the National Science Foundation. It is a pleasure to record my thanks to these organizations and especially to Dr. Geoffrey Keller, Dean of the College of Mathematics and Physical Sciences of the Ohio State University, and to Prof. C. de Jager, Assistant General Secretary of the International Astronomical Un ion, for their kind cooperation. I am also grateful to H. A. Abt, J. Hardorp, R. P. Kraft, Mrs. A. Massevitch, M. Plavec, 1. W. Roxburgh, and E. Schatzman of the Organizing Committee, as well as A. J. Deutsch and G. W. Collins, II, for their help in planning the Colloquium all of them offered valuable suggestions toward organizing the program.

The Rotation of Sun and Stars

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Author :
Publisher : Springer Science & Business Media
ISBN 13 : 3540878300
Total Pages : 266 pages
Book Rating : 4.5/5 (48 download)

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Book Synopsis The Rotation of Sun and Stars by : Jean-Pierre Rozelot

Download or read book The Rotation of Sun and Stars written by Jean-Pierre Rozelot and published by Springer Science & Business Media. This book was released on 2009-01-08 with total page 266 pages. Available in PDF, EPUB and Kindle. Book excerpt: The Sun and stars rotate in di?erent ways and at di?erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi?erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di?erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic ?eld is strongly linked to the matter motions in the solar plasma. The solar magnetic ?eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist – in any case magnetic ?eld and rotation cannot thus be separated.

Physics, Formation and Evolution of Rotating Stars

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Publisher : Springer Science & Business Media
ISBN 13 : 3540769498
Total Pages : 832 pages
Book Rating : 4.5/5 (47 download)

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Book Synopsis Physics, Formation and Evolution of Rotating Stars by : Andre Maeder

Download or read book Physics, Formation and Evolution of Rotating Stars written by Andre Maeder and published by Springer Science & Business Media. This book was released on 2008-12-19 with total page 832 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Studying Stellar Rotation and Convection

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Author :
Publisher : Springer
ISBN 13 : 364233380X
Total Pages : 265 pages
Book Rating : 4.6/5 (423 download)

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Book Synopsis Studying Stellar Rotation and Convection by : Mariejo Goupil

Download or read book Studying Stellar Rotation and Convection written by Mariejo Goupil and published by Springer. This book was released on 2012-12-15 with total page 265 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Understanding Stellar Evolution

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Author :
Publisher : CRC Press
ISBN 13 : 9780750312790
Total Pages : 342 pages
Book Rating : 4.3/5 (127 download)

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Book Synopsis Understanding Stellar Evolution by : Henny J. G. L. M. Lamers

Download or read book Understanding Stellar Evolution written by Henny J. G. L. M. Lamers and published by CRC Press. This book was released on 2018-02-28 with total page 342 pages. Available in PDF, EPUB and Kindle. Book excerpt: 'Understanding Stellar Evolution' is based on a series of graduate-level courses taught at the University of Washington since 2004, and is written for physics and astronomy students and for anyone with a physics background who is interested in stars. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between the different processes inside stars such as nuclear reactions, energy transport, chemical mixing, pulsation, mass loss, and rotation. Based on these principles, the evolution of low- and high-mass stars is explained from their formation to their death. In addition to homework exercises for each chapter, the text contains a large number of questions that are meant to stimulate the understanding of the physical principles. An extensive set of accompanying lecture slides is available for teachers in both Keynote(R) and PowerPoint(R) formats.

The Rotation of Sun and Stars

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Author :
Publisher : Springer
ISBN 13 : 9783540879275
Total Pages : 264 pages
Book Rating : 4.8/5 (792 download)

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Book Synopsis The Rotation of Sun and Stars by : Jean-Pierre Rozelot

Download or read book The Rotation of Sun and Stars written by Jean-Pierre Rozelot and published by Springer. This book was released on 2009-08-29 with total page 264 pages. Available in PDF, EPUB and Kindle. Book excerpt: The Sun and stars rotate in di?erent ways and at di?erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi?erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di?erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic ?eld is strongly linked to the matter motions in the solar plasma. The solar magnetic ?eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist – in any case magnetic ?eld and rotation cannot thus be separated.

Stellar Rotation

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Publisher :
ISBN 13 : 9780677601700
Total Pages : 356 pages
Book Rating : 4.6/5 (17 download)

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Book Synopsis Stellar Rotation by : Arne Slettebak

Download or read book Stellar Rotation written by Arne Slettebak and published by . This book was released on 1970-01-01 with total page 356 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology

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Author :
Publisher : Springer
ISBN 13 : 3319509896
Total Pages : 110 pages
Book Rating : 4.3/5 (195 download)

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Book Synopsis Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology by : Martin Bo Nielsen

Download or read book Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology written by Martin Bo Nielsen and published by Springer. This book was released on 2017-01-24 with total page 110 pages. Available in PDF, EPUB and Kindle. Book excerpt: In his PhD dissertation Martin Bo Nielsen performs observational studies of rotation in stars like the Sun. The interior rotation in stars is thought to be one of the driving mechanisms of stellar magnetic activity, but until now this mechanism was unconstrained by observational data. NASA’s Kepler space mission provides high-precision observations of Sun-like stars which allow rotation to be inferred using two independent methods: asteroseismology measures the rotation of the stellar interior, while the brightness variability caused by features on the stellar surface trace the rotation of its outermost layers. By combining these two techniques Martin Bo Nielsen was able to place upper limits on the variation of rotation with depth in five Sun-like stars. These results suggest that the interior of other Sun-like stars also rotate in much the same way as our own Sun.

Differential Rotation and Stellar Convection

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Author :
Publisher : Taylor & Francis
ISBN 13 : 9782881240669
Total Pages : 332 pages
Book Rating : 4.2/5 (46 download)

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Book Synopsis Differential Rotation and Stellar Convection by : Günther Rüdiger

Download or read book Differential Rotation and Stellar Convection written by Günther Rüdiger and published by Taylor & Francis. This book was released on 1989 with total page 332 pages. Available in PDF, EPUB and Kindle. Book excerpt: First Published in 1989. Routledge is an imprint of Taylor & Francis, an informa company.

Stellar Rotation

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Author :
Publisher : Springer
ISBN 13 : 9789027701565
Total Pages : 355 pages
Book Rating : 4.7/5 (15 download)

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Book Synopsis Stellar Rotation by : A. Slettebak

Download or read book Stellar Rotation written by A. Slettebak and published by Springer. This book was released on 1970-07-31 with total page 355 pages. Available in PDF, EPUB and Kindle. Book excerpt: The International Astronomical Union Colloquium on Stellar Rotation was held at the Ohio State University in Columbus, Ohio, U.S.A. from September 8th through 11 th, 1969. Forty-four scientists from Argentina, Belgium, Canada, England, Finland, East and West Germany, Italy, Israel, Japan, The Netherlands, and the United States attended and participated in the Colloquium. The present volume, which parallels the actual program closely, contains the papers presented at the Colloquium plus most of the discussion following those papers. The Colloquium was sponsored by the International Astronomical Union, the Ohio State University, and the National Science Foundation. It is a pleasure to record my thanks to these organizations and especially to Dr. Geoffrey Keller, Dean of the College of Mathematics and Physical Sciences of the Ohio State University, and to Prof. C. de Jager, Assistant General Secretary of the International Astronomical Un ion, for their kind cooperation. I am also grateful to H. A. Abt, J. Hardorp, R. P. Kraft, Mrs. A. Massevitch, M. Plavec, 1. W. Roxburgh, and E. Schatzman of the Organizing Committee, as well as A. J. Deutsch and G. W. Collins, II, for their help in planning the Colloquium all of them offered valuable suggestions toward organizing the program.

Rotating Relativistic Stars

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Publisher : Cambridge University Press
ISBN 13 : 1107310601
Total Pages : 435 pages
Book Rating : 4.1/5 (73 download)

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Book Synopsis Rotating Relativistic Stars by : John L. Friedman

Download or read book Rotating Relativistic Stars written by John L. Friedman and published by Cambridge University Press. This book was released on 2013-02-11 with total page 435 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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. (PSA-1), Volume 1

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Publisher : Princeton University Press
ISBN 13 : 140086898X
Total Pages : 524 pages
Book Rating : 4.4/5 (8 download)

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Book Synopsis Theory of Rotating Stars. (PSA-1), Volume 1 by : Jean-Louis Tassoul

Download or read book Theory of Rotating Stars. (PSA-1), Volume 1 written by Jean-Louis Tassoul and published by Princeton University Press. This book was released on 2015-03-08 with total page 524 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Theory of Rotating Stars

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Author :
Publisher :
ISBN 13 : 9780691082141
Total Pages : 506 pages
Book Rating : 4.0/5 (821 download)

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Book Synopsis Theory of Rotating Stars by : Jean Louis Tassoul

Download or read book Theory of Rotating Stars written by Jean Louis Tassoul and published by . This book was released on 1978 with total page 506 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

The Observation and Analysis of Stellar Photospheres

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Publisher : Cambridge University Press
ISBN 13 : 9780521851862
Total Pages : 560 pages
Book Rating : 4.8/5 (518 download)

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Book Synopsis The Observation and Analysis of Stellar Photospheres by : David F. Gray

Download or read book The Observation and Analysis of Stellar Photospheres written by David F. Gray and published by Cambridge University Press. This book was released on 2005-11-17 with total page 560 pages. Available in PDF, EPUB and Kindle. Book excerpt: Third edition textbook for use on advanced courses on stellar physics.

Stellar Rotation

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Publisher :
ISBN 13 :
Total Pages : 256 pages
Book Rating : 4.:/5 (17 download)

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Book Synopsis Stellar Rotation by : Jean Louis Tassoul

Download or read book Stellar Rotation written by Jean Louis Tassoul and published by . This book was released on 2000 with total page 256 pages. Available in PDF, EPUB and Kindle. Book excerpt: