2006/10/28 by F. Combes, S. García-Burillo, S. Garcia-Burillo +13 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #High resolution #Luminosity #Redshift #Star formation #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066559
4 pages, 5 figures, accepted A&A Letters, extended-PdB special issue
arxiv created 2006/10/28 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present the results of mapping the CO(1–0) emission of the ultra-luminous starburst IRAS 11582+3020, with the IRAM interferometer, at ~1´´ resolution. This galaxy was selected from an IRAM-30 m survey of 30 galaxies at moderate redshift () to explore galaxy evolution and, in particular, the efficiency of star formation, in the redshift range filling the gap between local and very high-z objects. The CO emission is kinematically resolved, and about 50% of the total emission found in the 27´´ (97 kpc) single dish beam is not recovered by the interferometer. This indicates that some extended emission may be present on large scales (typically 7–15´´). The FIR-to-CO luminosity ratio follows the trend from local to high-z ultra-luminous starbursts.