High Energy Astrophysics
by Jonathan Katz
Publisher: The Benjamin/Cummings Publishing 1986
Number of pages: 338
This book describes the ingredients, methods, and results of modern astrophysical phenomenology and modeling for advanced undergraduates or beginning graduate students. It is meant to be explanatory and expository, rather than complete or definitive.
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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 J. B. Tatum
A course on stellar atmospheres: radiation theory, blackbody radiation, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction, the equation of transfer, limb darkening, atomic spectroscopy, 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.
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.