by J. B. Tatum
A course on stellar atmospheres which covers: definitions of and relations between quantities used in radiation theory, blackbody radiation, the exponential integral function, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction and the equation of transfer, limb darkening, atomic spectroscopy, Boltzmann's and Saha's equations, oscillator strengths and related topics, line profiles, curve of growth.
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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 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 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.