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Simulating galaxy evolution

Name: Simulating galaxy evolution
Keywords: Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 1999Embargo end date: 01 Jan 1998Publisher:ASCEJournal:The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5)

Authors: Rychard Bouwens; Joseph Silk;

doi: 10.1063/1.58639 , 10.48550/arxiv.astro-ph/9812322

arXiv: http://arxiv.org/abs/astro-ph/9812322

Simulating galaxy evolution

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Abstract

The forwards approach to galaxy formation and evolution is extremely powerful but leaves several questions unanswered. Foremost among these is the origin of disks. A backwards approach is able to provide a more realistic treatment of star formation and feedback and provides a practical guide to eventually complement galaxy formation ab initio.

11 pages with 2 figures, to appear in "After the Dark Ages: When Galaxies were Young", proceedings of the 9th annual October Astrophysics Conference, ed. S. Holt and E. Smith, simulated images available at http://astro.berkeley.edu/~bouwens/simulation.html

Related Organizations

University of California, Berkeley
United States
University of California System
United States

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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NEANIAS Space Research Community