Stellar Structure and Evolution
by Sergey V. Vorontsov
Publisher: Queen Mary, University of London 2010
Contents: Introduction; 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.
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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.
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