THE BLACK HOLE MASSES AND STAR FORMATION RATES OF z > 1 DUST OBSCURED GALAXIES: RESULTS FROM KECK OSIRIS INTEGRAL FIELD SPECTROSCOPY

被引：22
作者：
Melbourne, J. [1 ]
Peng, Chien Y. [2 ]
Soifer, B. T. [1 ,3 ]
Urrutia, Tanya [3 ]
Desai, Vandana [3 ]
Armus, L. [3 ]
Bussmann, R. S. [4 ]
Dey, Arjun [5 ]
Matthews, K. [1 ]
机构：
[1] CALTECH, Caltech Opt Observ, Div Phys Math & Astron, Pasadena, CA 91125 USA
[2] Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7, Canada
[3] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[4] Univ Arizona, LBT Observ, Tucson, AZ 85721 USA
[5] Natl Opt Astron Observ, Tucson, AZ 85726 USA
来源：
ASTRONOMICAL JOURNAL | 2011年 / 141卷 / 04期
关键词：
black hole physics; galaxies: active; galaxies: high-redshift; instrumentation: adaptive optics; SIMILAR-TO; 2; ACTIVE GALACTIC NUCLEI; QUASAR HOST GALAXIES; ADAPTIVE OPTICS; HIGH-REDSHIFT; INFRARED GALAXIES; FORMING GALAXIES; SPACE-TELESCOPE; MORPHOLOGIES; COEVOLUTION;
D O I：
10.1088/0004-6256/141/4/141
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have obtained high spatial resolution Keck OSIRIS integral field spectroscopy of four z similar to 1.5 ultra-luminous infrared galaxies that exhibit broad H alpha emission lines indicative of strong active galactic nucleus (AGN) activity. The observations were made with the Keck laser guide star adaptive optics system giving a spatial resolution of 0 ''.1 or <1 kpc at these redshifts. These high spatial resolution observations help to spatially separate the extended narrow-line regions-possibly powered by star formation-from the nuclear regions, which may be powered by both star formation and AGN activity. There is no evidence for extended, rotating gas disks in these four galaxies. Assuming dust correction factors as high as A(H alpha) = 4.8 mag, the observations suggest lower limits on the black hole masses of (1-9) x 10(8) M-circle dot and star formation rates < 100 M-circle dot yr(-1). The black hole masses and star formation rates of the sample galaxies appear low in comparison to other high-z galaxies with similar host luminosities. We explore possible explanations for these observations, including host galaxy fading, black hole growth, and the shut down of star formation.
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页数：11
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