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 Sergey V. Vorontsov - Queen Mary, University of London
Contents: 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.
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 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 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.