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Hierarchical, dissipative formation of elliptical galaxies: is thermal instability the key mechanism? Hydrodynamical simulations including supernova feedback, multi-phase gas and metal enrichment in CDM: structure and dynamics of elliptical galaxies
Uppsala University.
Uppsala University.
1999 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 347, no 3, 769-798 p.Article in journal (Other scientific) Published
Abstract [en]

We present numerical simulations of galaxy formation, including star formation, in a standard, hierarchical cosmological scenario (CDM). The gas dynamics is followed with the Smooth Particle Hydrodynamics (SPH) method, and the gravitational interaction wi

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1999. Vol. 347, no 3, 769-798 p.
Keyword [en]
hydrodynamics; methods : numerical; galaxies : elliptical and lenticular; cD; galaxies : formation; galaxies : structure; STAR-FORMING GALAXIES; COLD DARK MATTER; REDSHIFTS Z-GREATER-THAN-3; COSMOLOGICAL CONTEXT; GLOBULAR-CLUSTERS; HUBBLE SEQUENCE; BAADES
URN: urn:nbn:se:uu:diva-85274OAI: oai:DiVA.org:uu-85274DiVA: diva2:113182
Addresses: Pharasyn A, Uppsala Astron Observ, Box 515, S-75120 Uppsala, Sweden. Uppsala Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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ReferencesLink to record
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