A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures across Cosmic Time

被引:15
作者
Imara, Nia [1 ]
Loeb, Abraham [1 ]
Johnson, Benjamin D. [1 ]
Conroy, Charlie [1 ]
Behroozi, Peter [2 ,3 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[2] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
关键词
dark ages; reionization; first stars; dust; extinction; early universe; galaxies: evolution; galaxies: high-redshift; DARK-MATTER HALO; METALLICITY RELATION; INTERSTELLAR DUST; INFRARED-EMISSION; STELLAR EVOLUTION; ANGULAR-MOMENTUM; DWARF GALAXIES; GAS FRACTIONS; DISK GALAXIES; DEEP FIELD;
D O I
10.3847/1538-4357/aaa3f0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the evolution of dust content in galaxies from redshifts z = 0 to z = 9.5. Using empirically motivated prescriptions, we model galactic-scale properties-including halo mass, stellar mass, star formation rate, gas mass, and metallicity-to make predictions for the galactic evolution of dust mass and dust temperature in main-sequence galaxies. Our simple analytic model, which predicts that galaxies in the early universe had greater quantities of dust than their low-redshift counterparts, does a good job of reproducing observed trends between galaxy dust and stellar mass out to z approximate to 6. We find that for fixed galaxy stellar mass, the dust temperature increases from z = 0 to z = 6. Our model forecasts a population of low-mass, high-redshift galaxies with interstellar dust as hot as, or hotter than, their more massive counterparts; but this prediction needs to be constrained by observations. Finally, we make predictions for observing 1.1 mm flux density arising from interstellar dust emission with the Atacama Large Millimeter Array.
引用
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页数:15
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