Where stars form and live at high redshift: clues from the infrared

被引:33
作者
Bethermin, M. [1 ,2 ,3 ,4 ]
Dore, O. [5 ]
Lagache, G. [2 ,3 ,4 ]
机构
[1] Univ Paris Diderot, CNRS, Lab AIM Paris Saclay, CEA,DSM,Irfu, Saclay, France
[2] Inst Astrophys Spatiale IAS, F-91405 Orsay, France
[3] Univ Paris 11, Paris, France
[4] CNRS, UMR8617, F-75700 Paris, France
[5] CALTECH, Jet Prop Lab, Pasadena, CA USA
来源
ASTRONOMY & ASTROPHYSICS | 2012年 / 537卷
关键词
galaxies: star formation; galaxies: statistics; galaxies: halos; dark matter; infrared: galaxies; STELLAR MASS FUNCTION; LESS-THAN; 2; HALO MASS; LUMINOSITY FUNCTION; GAS CLOUDS; GALAXIES; EVOLUTION; FRAGMENTATION; MORPHOLOGY; SAMPLE;
D O I
10.1051/0004-6361/201118607
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The relation between dark matter halos and the loci of star formation at high redshift is a pressing question in contemporary cosmology. Matching the abundance of halos to the abundance of infrared (IR) galaxies, we explore the link between dark matter halo mass (M-h), stellar mass (M-*) and star-formation rate (SFR) up to a redshift of 2. Our findings are five-fold. First, we find a strong evolution of the relation between M-* and SFR as a function of redshift with an increase of sSFR = SFR/M-* by a factor similar to 30 between z = 0 and z = 2.3. Second, we observe a decrease of sSFR with stellar mass. These results reproduce observed trends at redshift z > 0.3. Third, we find that the star formation is most efficient in dark matter halos with M-h similar or equal to 5 x 10(11) M-circle dot, with hints of an increase of this mass with redshift. Fourth, we find that SFR/M-h increases by a factor similar to 15 between z = 0 and z = 2.3. Finally we find that the SFR density is dominated by halo masses close to similar to 7 x 10(11) M-circle dot at all redshift, with a rapid decrease at lower and higher halo masses. Despite its simplicity, our novel use of IR observations unveils some characteristic mass-scales governing star formation at high redshift.
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页数:4
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