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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- 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 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.
by Simon C. O. Glover - arXiv
The author discusses our current understanding of the physical processes involved in the formation of Population III stars. He shows how we can identify the mass scale of the first dark matter halos to host Population III star formation.
by George W. Collins, II - Pachart Pub. House
The virial theorem is extremely powerful in understanding problems of stellar astrophysics, but it is also poorly understood by many who study the subject. This book should be viewed as a guided introduction, punctuated by a few examples.