Studying the complex physical systems of stellar jets
necessitates the incorporation of nonlinear effects which occur on
a wide variety of length and timescales. One of the primary methods
used to study the physics of jets is numerical simulations that
apply high performance computing techniques. Such techniques are
also required for analysing the huge modern astrophysical
datasets.
This book examines those computing techniques. It is a
collection of the lectures from the fifth and final school of the
JETSET network, "Jets From Young Stars V: High Performance
Computing in Astrophysics." It begins with an introduction to
parallel programming techniques, with an emphasis on Message
Passing Interface (MPI), before it goes on to review grid
technology techniques and offer a practical introduction to Virtual
Observatory. The second half of the book, then, is devoted to
applications of high performance computing techniques, including 3D
radiation transfer, to jet and star formation processes.
Aimed at graduate students in astrophysics, this book presents
state-of-the-art methods, thereby offering interesting new insights
to researchers in the field.
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