A Practical Introduction to Numerical Hydrodynamics
by Garrelt Mellema
Publisher: Leiden University 2003
This text is an introduction to the field of numerical hydrodynamics. It will hopefully 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, but this type of models could also apply to for instance galaxies, their cores, disks, and even clusters.
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by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl - arXiv
The authors focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis on the composition of their ejecta in form of stellar winds during the evolution or of explosive ejecta.
- 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 James N. Pierce - Minnesota State University
This book provides an introduction to the details of the structure, operation, and evolution of stars. It will be most useful to undergraduates in upper-level astronomy courses and graduate students taking Stellar Interiors or Stellar Atmospheres.
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.