Herschel☆-ATLAS: properties of dusty massive galaxies at low and high redshifts

被引：60

作者：

Rowlands, K. ^{[1
,2
]}

Dunne, L. ^{[3
]}

Dye, S. ^{[1
]}

Aragon-Salamanca, A. ^{[1
]}

Maddox, S. ^{[3
]}

da Cunha, E. ^{[4
]}

Smith, D. J. B. ^{[5
]}

Bourne, N. ^{[1
,6
]}

Eales, S. ^{[7
]}

Gomez, H. L. ^{[7
]}

Smail, I. ^{[8
]}

Alpaslan, M. ^{[2
,9
]}

Clark, C. J. R. ^{[7
]}

Driver, S. ^{[2
,9
]}

Ibar, E. ^{[10
]}

Ivison, R. J. ^{[6
,11
]}

Robotham, A. ^{[2
,9
]}

Smith, M. W. L. ^{[7
]}

Valiante, E. ^{[7
]}

机构：

[1] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England

[2] Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[3] Univ Canterbury, Dept Phys & Astron, Christchurch 1, New Zealand

[4] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[5] Univ Hertfordshire, Sci & Technol Res Inst, Ctr Astrophys, Hatfield AL10 9AB, Herts, England

[6] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland

[7] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[8] Univ Durham, Inst Computat Cosmol, Dept Phys, Durham DH1 3LE, England

[9] Univ Western Australia, Int Ctr Radio Astron ICRAR, Crawley, WA 6009, Australia

[10] Univ Valparaiso, Inst Fis & Astron, Valparaiso 2360102, Chile

[11] European So Observ, D-85748 Garching, Germany

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2014年 / 441卷 / 02期

基金：

欧洲研究理事会;

关键词：

dust; extinction; galaxies: evolution; galaxies: fundamental parameters; galaxies: high-redshift; galaxies: ISM; submillimetre: galaxies; STAR-FORMING GALAXIES; DEEP-FIELD-SOUTH; GOODS-N FIELD; SUBMILLIMETER-SELECTED GALAXIES; SCIENCE DEMONSTRATION PHASE; HERSCHEL REFERENCE SURVEY; FAR-INFRARED PROPERTIES; SPECTRAL ENERGY-DISTRIBUTIONS; CO-TO-H-2 CONVERSION FACTOR; DEGREE EXTRAGALACTIC SURVEY;

D O I：

10.1093/mnras/stu510

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a comparison of the physical properties of a rest-frame 250-mu m-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature and 843 dusty galaxies at z < 0.5 from the Herschel-Astrophysical TeraHertz Large Area Survey (H-ATLAS), selected to have a similar stellar mass to the SMGs. The z > 1 SMGs have an average star formation rate (SFR) of 390(-70)(+80) M-circle dot yr(-1), which is 120 times that of the low-redshift sample matched in stellar mass to the SMGs (SFR = 3.3 +/- 0.2 M-circle dot yr(-1)). The SMGs harbour a substantial mass of dust (1.2(-0.2)(+0.3) x 10(9) M-circle dot), compared to (1.6 +/- 0.1) x 10(8) M-circle dot for low-redshift dusty galaxies. At low redshifts, the dust luminosity is dominated by the diffuse interstellar medium, whereas a large fraction of the dust luminosity in SMGs originates from star-forming regions. At the same dust mass, SMGs are offset towards a higher SFR compared to the low-redshift H-ATLAS galaxies. This is not only due to the higher gas fraction in SMGs but also because they are undergoing a more efficient mode of star formation, which is consistent with their bursty star formation histories. The offset in SFR between SMGs and low-redshift galaxies is similar to that found in CO studies, suggesting that dust mass is as good a tracer of molecular gas as CO.

引用

页码：1017 / 1039

页数：23

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