Publisher: Wikipedia 2014
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.
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by George W. Collins, II - W H Freeman & Co
The book on stellar astrophysics for the first year graduates or the advanced undergraduate students. It is assumed that the readers have factual knowledge of stars and astronomy. The text describes the axiomatic theory of stellar structure.
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
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.
by J. B. Tatum
A course on stellar atmospheres: radiation theory, blackbody radiation, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction, the equation of transfer, limb darkening, atomic spectroscopy, and more.