Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality
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Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality

Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality


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About the Book

Physical Processes in the Interstellar Medium.- Introduction.- Composition of the ISM.- Heating and cooling of interstellar gas.- ISM Turbulence.- Formation of molecular clouds.- Star Formation.- Summary.- High performance computing and numerical modelling.- Preamble.- Collisionless N-Body dynamics.- Time Integration techniques.- Gravitationals force calculation.- Basic gas dynamics.- Eularian hydrodynamics.- Smoothed particle hydrodynamics.- Moving-mesh techniques.- Parallelized techniques and current computing Trends.-


About the Author: Nick Gnedin is a research scientist at the Fermi National Accelerator Laboratory and a professor at the University of Chicago. He is a Fellow of the American Physical Society.
Volker Springel is professor for theoretical astrophysics at Heidelberg University, Germany. He leads a research group in numerical cosmology at the Heidelberg Institute for Theoretical Studies.
Ralf S. Klessen is professor for theoretical astrophysics at the Center for Astronomy of Heidelberg University. He works on various aspects of stellar birth in the early universe as well as at present days, and he studies the dynamics of the interstellar medium.
Simon Glover is a researcher in the Centre for Astronomy at Heidelberg University. His research focuses on the influence of chemical and radiative processes on the formation of stars and galaxies.


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Product Details
  • ISBN-13: 9783662516768
  • Publisher: Springer
  • Binding: Paperback
  • Height: 234 mm
  • No of Pages: 365
  • Series Title: Saas-Fee Advanced Course
  • Sub Title: Saas-Fee Advanced Course 43. Swiss Society for Astrophysics and Astronomy
  • Width: 156 mm
  • ISBN-10: 3662516764
  • Publisher Date: 25 Oct 2016
  • Edition: Softcover reprint of the original 1st ed. 2015
  • Language: English
  • Returnable: N
  • Spine Width: 20 mm
  • Weight: 580 gr


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Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality
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