This book is a quantitative introduction to what is known or theorized about the structure and evolution of galactic systems. It begins with a general introduction to galaxies and a summary of our empirical observations of galaxies in the universe, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is then covered. The book concludes with a discussion of the...

This textbook gives a clear account of the manner in which knowledge in many branches of physics, such as gravitation, thermodynamics, atomic physics, and nuclear physics, can be combined to gain an understanding of the structure and evolution of stars. A major aim is to present the subject as one in which advances are still being made. The first half is an account of the observational properties of stars and a discussion of the equations that govern their structure. The second part discusses recent theoretical work on stellar evolution. The successes of the theory are stressed, but attention...

Using mathematics appropriate for advanced undergraduate students in physics, this textbook provides a broad and wide-ranging introduction to the Sun as a star. Tayler provides succinct derivations of key results--such as the properties of spectral lines, the theory of stellar oscillations, plasma physics, magnetohydrodynamics and dynamo theory--in nine handy appendices, ensuring that the book is completely self contained. Altogether, this is an invaluable textbook for students studying the Sun, stars, the solar-terrestrial environment and the formation of planetary systems.

Using mathematics appropriate for advanced undergraduate students in physics, this textbook provides a broad and wide-ranging introduction to the Sun as a star. Tayler provides succinct derivations of key results--such as the properties of spectral lines, the theory of stellar oscillations, plasma physics, magnetohydrodynamics and dynamo theory--in nine handy appendices, ensuring that the book is completely self contained. Altogether, this is an invaluable textbook for students studying the Sun, stars, the solar-terrestrial environment and the formation of planetary systems.

Viele Zweige der Physik wie Gravitation, Thermodynamik, Atomphysik und Kernphysik tragen zur Bestimmung des inneren Aufbaus der Sterne bei. Die physikalischen Bedingungen sind in Sternen extremer als auf der Erde. Eine erfolgreiche Erforschung ihres Aufbaus sollte zeigen, in wieweit man die auf der Erde erprobten physikalischen Gesetze auf diese Bedingungen extrapolieren kann. Ein beachtlicher Fortschritt konnte bei der Erklarung der beobachteten Eigenschaften der Sterne bereits erzielt werden, viele Beobachtungen kannen aber noch nicht vollstandig gedeutet werden. Ein Hauptanliegen dieses...