Star formation rate and metallicity of damped Lyman α absorbers in cosmological smoothed particle hydrodynamics simulations

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 2, 2004, Pages 435-450

  Nagamine, K ^a   Springel, V ^b   Hernquist, L ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: theory; Galaxies: evolution; Galaxies: formation; Methods: numerical

Indexed keywords

GALAXIES; HYDRODYNAMICS; METALS; NUMERICAL METHODS; SUPERNOVAE;

COSMOLOGY: THEORY; GALAXY EVOLUTION; GALAXY FORMATIONS; HYDRODYNAMIC SIMULATION; METALLICITIES; METHOD: NUMERICAL; RED SHIFT; REDSHIFT RANGE; SMOOTHED PARTICLE HYDRODYNAMICS; STAR FORMATION RATES;

COSMOLOGY;

EID: 1442359761     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07180.x     Document Type: Article

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