Massive Stars and their Supernovae
by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl
Publisher: arXiv 2010
Number of pages: 81
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).
Home page url
Download or read it online for free here:
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 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.
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.
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.