uu.seUppsala University Publications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Cooling limits on galaxy formation - Gas dynamical simulations incorporating a background UV field and metal enrichment
Uppsala University.
Uppsala University.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 333, no 2, 399-410 p.Article in journal (Other scientific) Published
Abstract [en]

We present hydrodynamical simulations of the formation of galaxies in the mass range 10(9) - 10(13)M., with the focus on the efficiency of gas cooling. The effect of a background UV radiation field, and the effect of metal enrichment of halo gas due to st

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 333, no 2, 399-410 p.
Keyword [en]
galaxies : formation; cooling flows; hydrodynamics; methods : numerical; ANGULAR-MOMENTUM; ALPHA CLOUDS; DARK HALOS; FRAGMENTATION; REDSHIFT; COLLAPSE; PEAKS
Identifiers
URN: urn:nbn:se:uu:diva-85310OAI: oai:DiVA.org:uu-85310DiVA: diva2:113218
Note
Addresses: Hultman J, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

Open Access in DiVA

No full text

By organisation
Uppsala University

Search outside of DiVA

GoogleGoogle Scholar

urn-nbn

Altmetric score

urn-nbn
Total: 443 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf