The Birth and Death of Stars
by James Schombert
Publisher: University of Oregon 2008
Stars are directly, or indirectly, the source of all the energy necessary to sustain life on our world. This course will study the birth, evolution and death of stars in the Milky Way galaxy, with a particular emphasis on the underlying science behind stellar and galactic evolution, the observational aspect to astronomy and our knowledge of how the Universe operates on the stellar scale.
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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.
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 P.K. Townsend - arXiv
Notes for a course taught in part III of the Cambridge University Mathematical Tripos: gravitational collapse, Schwarzschild black hole, charged black holes; rotating black holes; energy and angular momentum; black hole mechanics; Hawking radiation.
by Jonathan Katz - The Benjamin/Cummings Publishing
This book describes the methods and results of modern astrophysical phenomenology and modelling for advanced undergraduates or beginning graduate students. It is meant to be explanatory and expository, rather than complete or definitive.