The nature of submillimetre galaxies in cosmological hydrodynamic simulations

Monthly Notices of the Royal Astronomical Society

Volumn 404, Issue 3, 2010, Pages 1355-1368

  Davé, Romeel ^a   Finlator, Kristian ^a,b   Oppenheimer, Benjamin D ^a,c   Fardal, Mark ^d   Katz, Neal ^d   Kereš, Dušan ^e   Weinberg, David H ^f  

^a UNIVERSITY OF ARIZONA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c LEIDEN UNIVERSITY   (Netherlands)

^d UNIVERSITY OF MASSACHUSETTS   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f OHIO STATE UNIVERSITY   (United States)

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: starburst; Methods: N body simulations; Submillimetre

Indexed keywords

GALAXIES; HYDRODYNAMICS; STARS;

CLUSTERINGS; GALAXIES: STARBURSTS; GALAXIES:HIGH-REDSHIFT; GALAXY EVOLUTION; GALAXY FORMATIONS; HYDRODYNAMIC SIMULATION; METHODS:N-BODY SIMULATIONS; STAR FORMATION RATES; SUBMILLIMETER: GALAXIES; SUBMILLIMETRE;

COSMOLOGY;

EID: 77952920730     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16395.x     Document Type: Article

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