CO line emission from Lyman break galaxies: Cosmological simulations and predictions for ALMA

Astronomy and Astrophysics

Volumn 480, Issue 2, 2008, Pages 335-338

  Greve, T R ^a,b   Sommer Larsen, J ^c  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c Dark Cosmology Centre   (Denmark)

Author keywords

Cosmology: theory; Galaxies: formation; ISM: molecules; Methods: N body simulations

Indexed keywords

COSMOLOGY; DENSITY (SPECIFIC GRAVITY); GALAXIES; MORPHOLOGY; PHYSICAL PROPERTIES; SPECTRAL RESOLUTION;

COSMOLOGY: THEORY; GALAXIES: FORMATION; ISM: MOLECULES; METHODS: N-BODY SIMULATIONS;

CARBON MONOXIDE;

EID: 41449087389     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078013     Document Type: Article

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