Protostars and Planets
Publisher: Rice University 2015
Number of pages: 422
The book describes the very rapidly growing area of star-and-planet formation and evolution. The text covers everything from astrophysics to planetary science, spanning the parsec-sized molecular clouds down to the formation of microscopic inclusions in meteorites in the early solar system. It is most useful for researchers, graduate students, and some undergraduate students.
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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 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.
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Investigations of the heating of the corona and the acceleration of the solar wind are two of the prime scientific goals in studying the solar upper atmosphere with the Solar and Heliospheric Observatory (SOHO) of ESA and NASA.
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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.