Stellar Structure and Evolution
by Sergey V. Vorontsov
Publisher: Queen Mary, University of London 2010
Contents: Introduction; Basic observational data; Equation of state: the ideal gas; Hydrostatic equilibrium; Polytropic models; Nuclear energy generation; Energy transport by radiation; Energy transport by convection; Evolution after the main sequence.
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by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl - arXiv
The authors focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis on the composition of their ejecta in form of stellar winds during the evolution or of explosive ejecta.
A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating as much energy as the Sun or any ordinary star is expected to emit over its entire life span, before fading from view over several weeks or months.
by James Schombert - University of Oregon
This course studies the birth, evolution and death of stars in our galaxy, emphasizing the underlying science behind stellar and galactic evolution, the observational aspect and our knowledge of how the Universe operates on the stellar scale.
by George W. Collins, II - Pachart Pub. House
The virial theorem is extremely powerful in understanding problems of stellar astrophysics, but it is also poorly understood by many who study the subject. This book should be viewed as a guided introduction, punctuated by a few examples.