Author: Matthias Bartelmann
Paperback: 340 pages
Publisher: Wiley-VCH; 1 edition (January 29, 2013)
Language: English
ISBN-10: 352741004X
ISBN-13: 978-3527410040
Format: Retail PDF
Reader Required: Adobe Reader, Foxit, Nitro, Adobe Digital Editions

Note: This is the eBook of the printed book and may not include any media, website access codes, or print supplements that may come packaged with the bound book.

Tested on the above readers with no problems on laptop and Android tablet.  Please allow a couple seconds for the seedboxes to kick in, then it should move pretty quick.
Hope it helps in your studies. Go for it! :D

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Beginning from first principles and adopting a modular structure, this book develops the fundamental physical methods needed to describe and understand a wide range of seemingly very diverse astrophysical phenomena and processes. For example, the discussion of radiation processes including their spectra is based on Larmor's equation and extended by the photon picture and the internal dynamics of radiating quantum systems, leading to the shapes of spectral lines and the ideas of radiation transport. Hydrodynamics begins with the concept of phase-space distribution functions and Boltzmann's equation and develops ideal, viscous and magneto-hydrodynamics all from the vanishing divergence of an energy-momentum tensor, opening a natural extension towards relativistic hydrodynamics. Linear stability analysis is introduced and used as a common and versatile tool throughout the book. 
Aimed at students at graduate level, lecturers teaching courses in theoretical astrophysics or advanced topics in modern astronomy, this book with its abundant examples and exercises also serves as a reference and an entry point for more advanced researchers wanting to update their knowledge of the physical processes that govern the behavior and evolution of astronomical objects.