資料來源: Google Book

Stellar rotation

  • 作者: Tassoul, Jean Louis.
  • 出版: Cambridge ;New York : Cambridge University Press 2000.
  • 稽核項: 1 online resource (xv, 256 pages) :illustrations.
  • 叢書名: Cambridge astrophysics series ;36
  • 標題: SCIENCE Astronomy. , Stars , SCIENCE , Rotation. , Astronomy. , Stars Rotation. , Étoiles , Electronic books. , Étoiles Rotation.
  • ISBN: 0521037697 , 9780521037693
  • ISBN: 0521772184
  • 試查全文@TNUA:
  • 附註: Includes bibliographical references and indexes. Preliminaries; Contents; Preface; 1 Observational basis; 2 Rotating fluids; 3 Rotating stars; 4 Meridional circulation; 5 Solar rotation; 6 The early-type stars; 7 The late-type stars; 8 Tidal interaction; Epilogue; Subject index; Author index
  • 摘要: 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.
  • 電子資源: https://dbs.tnua.edu.tw/login?url=https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=72928
  • 系統號: 005299446
  • 資料類型: 電子書
  • 讀者標籤: 需登入
  • 引用網址: 複製連結
Understanding how stars rotate is central to modeling their structure, formation and evolution, as well as understanding how they interact with their environment and companion stars. This lucid introduction to stellar rotation combines theory and observation, and includes all the latest developments in the field. Jean-Louis Tassoul, a leading authority on the subject, comprehensively surveys how the rotation of stars affects the structure and evolution of the Sun, single stars, and close binaries. This volume will greatly interest 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.
來源: Google Book
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