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Stellar rotation / / Jean-Louis Tassoul [[electronic resource]]



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Autore: Tassoul Jean Louis Visualizza persona
Titolo: Stellar rotation / / Jean-Louis Tassoul [[electronic resource]] Visualizza cluster
Pubblicazione: Cambridge : , : Cambridge University Press, , 2000
Descrizione fisica: 1 online resource (xv, 256 pages) : digital, PDF file(s)
Disciplina: 523.8
Soggetto topico: Stars - Rotation
Note generali: Title from publisher's bibliographic system (viewed on 05 Oct 2015).
Nota di bibliografia: Includes bibliographical references and indexes.
Nota di contenuto: 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
Sommario/riassunto: 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.
Titolo autorizzato: Stellar rotation  Visualizza cluster
ISBN: 1-107-11958-8
0-511-00963-1
1-280-42126-6
9786610421268
0-511-17254-0
0-511-15136-5
0-511-30206-1
0-511-54604-1
0-511-04969-2
Formato: Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione: Inglese
Record Nr.: 9910780072203321
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
Serie: Cambridge astrophysics series ; ; 36.