The rapid advance of computer capabilities over the last two
decades has opened up a new field of numerical simulations in which
detailed physical models can be made to represent the most complex
processes. IAU Symposium 270 reviews a wide range of topics
relevant to computer modeling in the fields of interstellar gas
dynamics, star formation and galactic dynamics. It includes
numerical techniques for modeling physical processes such as
self-gravitating, radiative magnetohydrodynamics, as well as novel
hardware options for acceleration and a view into the future of
computation. Observations of interstellar gas and star formation
are also reviewed. This book is ideal for graduate students and
researchers in the field of numerical astrophysics.
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