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Theory of Rotating Stars. (PSA-1), Volume 1

Jean-Louis Tassoul

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Naturwissenschaften, Medizin, Informatik, Technik / Naturwissenschaften allgemein

Beschreibung

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.

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Schlagwörter

Convection, Newton's law of universal gravitation, Variable star, Hyades (star cluster), Cosmogony, Stellar dynamics, Astronomy, Equation of state, Gravitational wave, Peculiar star, Galaxy rotation curve, The Astronomical Journal, Orbital plane (astronomy), Virial theorem, Star formation, Stellar atmosphere, Polytrope, Solar rotation, Stellar evolution, The Astrophysical Journal, Kepler's laws of planetary motion, Equation, Orbital period, Stellar rotation, Angular momentum, Chromosphere, G-type main-sequence star, Angular velocity, Planet, Stellar magnetic field, Lagrangian (field theory), Flare star, Orbit, Solar physics, Rotation period, Center of mass (relativistic), Main sequence, Sunspot, Formation and evolution of the Solar System, Gravitational constant, Planetary system, Spherical model, Gravitational potential, Be star, Cataclysmic variable star, Magnetic field, Boltzmann equation, White dwarf, Stellar structure, Galactic plane, Am star, Supernova, Spheroid, General relativity, Supergiant, Cosmic ray, Neutron star, Viscosity, Radiation pressure, Binary star, Quantity, Protostar, Variational method (quantum mechanics), Stellar density, T Tauri star, Differential rotation, Calculation, Cross section (physics), Cepheid variable, Roche limit