Simulating Galaxy Formation

dc.creatorSteinmetz, Matthias
dc.date1995-12-04
dc.date.accessioned2026-07-07T02:20:31Z
dc.date.available2026-07-07T02:20:31Z
dc.descriptionA review on numerical simulations of galaxy formation is given. Different numerical methods to solve collisionless and gas dynamical systems are outlined and one particular simulation technique, Smoothed Particle Hydrodynamics, is discussed in some detail. After a short discussion of the most relevant physical processes which affect the dynamics of the gas, the success and shortcomings of state of the art simulations are discussed via the example of the formation of disk galaxies.
dc.description24 pages, uuencoded postscript file, 5 figures, 2 figures included Proc. ``International School of Physics Enrico Fermi'', Course CXXXII: Dark Matter in the Universe, Varenna 1995, eds.: S. Bonometto, J. Primack, A. Provenzale, IOP, to appear; complete version available at http://www.mpa-garching.mpg.de/Galaxien/prep.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9512013
dc.identifierhttp://arxiv.org/abs/astro-ph/9512013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10235
dc.subjectAstrophysics
dc.titleSimulating Galaxy Formation
dc.typetext

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