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 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 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.
by Andreas Schmitt - arXiv
Cold and dense nuclear and quark matter can be found in the interior of compact stars. The author gives a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD.
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.