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 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.
- Rice University
This 1400+ pages book covers the very rapidly growing area of star-and-planet formation and evolution, from astrophysics to planetary science. It is most useful for researchers, graduate students, and some undergraduate students.
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.