Review
'... written with exceptional clarity ... the hallmark of Padmanabhan's work ... The mathematical derivations are elegant often starting from action principles, and readers may be enlightened by some which differ from standard approaches ... it is a magnificent achievement and a superb book.' Alan Heavens, The Observatory
'... the book develops a solid understanding of central concepts including stellar structure and evolution, the physics of stellar remnants such as while dwarfs and black holes, pulsars, binary stars, the sun and planetary systems, interstellar medium and globular clusters ... This indispensable volume provides graduate students with a self-contained introduction to stellar physics, and will allow them to master the material sufficiently to read and engage in research with heightened understanding.' Europe & Astronomy
'The book should not be missing in any astrophysical library.' Claudia-Veronika Meister, Zbl. MATH
Book Description
This second volume of a comprehensive three-volume course on theoretical astrophysics deals with stellar physics. Designed to help graduate students and researchers develop an understanding of the key physical processes governing stars and stellar systems, it teaches the fundamentals, and then builds on them to give the reader an in-depth understanding of advanced topics. It can be used alone or in conjunction with Volumes I and III (on astrophysical processes and on galaxies and cosmology, respectively). After reviewing the key observational results and nomenclature used in stellar astronomy, the book discusses stellar structure and evolution, the physics of stellar remnants, pulsars, binary stars, the sun and planetary systems, interstellar medium and globular clusters. More than seventy-five exercises test the reader's understanding.