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18 April 2024
 
  » arxiv » astro-ph/0502246

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Towards an understanding of the rapid decline of the cosmic star formation rate
Eric F. Bell ; Casey Papovich ; Christian Wolf ; Emeric Le Floc’h ; John A. R. Caldwell ; Marco Barden ; Eiichi Egami ; Daniel H. McIntosh ; Klaus Meisenheimer ; Pablo G. P. Perez-Gonzalez ; George H. Rieke ; Marcia J. Rieke ; Jane R. Rigby ; Hans-Walter Rix ;
Date 12 Feb 2005
Journal Astrophys.J. 625 (2005) 23-36
Subject astro-ph
AbstractWe present a first analysis of deep 24 micron observations with the Spitzer Space Telescope of a sample of nearly 1500 galaxies in a thin redshift slice, 0.652x10^10 solar masses) are undergoing a period of intense star formation above their past-averaged SFR. In contrast, less than 1% of equally-massive galaxies in the local universe have similarly intense star formation activity. Morphologically-undisturbed galaxies dominate the total infrared luminosity density and SFR density: at z~0.7, more than half of the intensely star-forming galaxies have spiral morphologies, whereas less than ~30% are strongly interacting. Thus, a decline in major-merger rate is not the underlying cause of the rapid decline in cosmic SFR since z~0.7. Physical properties that do not strongly affect galaxy morphology - for example, gas consumption and weak interactions with small satellite galaxies - appear to be responsible.
Source arXiv, astro-ph/0502246
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