Protostars and Planets
Publisher: Rice University 2015
Number of pages: 422
The book describes the very rapidly growing area of star-and-planet formation and evolution. The text covers everything from astrophysics to planetary science, spanning the parsec-sized molecular clouds down to the formation of microscopic inclusions in meteorites in the early solar system. It is most useful for researchers, graduate students, and some undergraduate students.
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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.
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 Gerard 't Hooft - Utrecht University
Contents: The Metric of Space and Time; Curved coordinates; A short introduction to General Relativity; Gravity; The Schwarzschild Solution; The Chandrasekhar Limit; Gravitational Collapse; The Reissner-Nordstrom Solution; Horizons; and more.
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.