A CORRELATION BETWEEN STAR FORMATION RATE AND AVERAGE BLACK HOLE ACCRETION IN STAR-FORMING GALAXIES

被引：158

作者：

Chen, Chien-Ting J. ^{[1
]}

Hickox, Ryan C. ^{[1
]}

Alberts, Stacey ^{[2
]}

Brodwin, Mark ^{[3
]}

Jones, Christine ^{[4
]}

Murray, Stephen S. ^{[5
]}

Alexander, DavidM. ^{[6
]}

Assef, Roberto J. ^{[7
]}

Brown, Michael J. I. ^{[8
]}

Dey, Arjun ^{[9
]}

Forman, William R. ^{[4
]}

Gorjian, Varoujan ^{[7
]}

Goulding, Andrew D. ^{[4
]}

Le Floc'h, Emeric ^{[10
]}

Jannuzi, Buell T. ^{[9
]}

Mullaney, James R. ^{[6
,10
]}

Pope, Alexandra ^{[2
]}

机构：

[1] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA

[2] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[3] Univ Missouri, Dept Phys & Astron, Kansas City, MO 64110 USA

[4] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[5] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[6] Univ Durham, Dept Phys, Durham DH1 3LE, England

[7] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[8] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia

[9] Natl Opt Astron Observ, Tucson, AZ 85726 USA

[10] Univ Paris Diderot, Lab AIM Paris Saclay, CEA, DSM,Irfu,CNRS,CE Saclay, F-91191 Gif Sur Yvette, France

来源：

ASTROPHYSICAL JOURNAL | 2013年 / 773卷 / 01期

关键词：

galaxies: active; galaxies: evolution; galaxies: starburst; infrared: galaxies; X-rays: galaxies; ACTIVE GALACTIC NUCLEI; SPECTRAL ENERGY-DISTRIBUTIONS; FORMATION RATE INDICATOR; QUASAR HOST GALAXIES; IRAC SHALLOW SURVEY; WIDE-FIELD SURVEY; SIMILAR-TO; 2.5; X-RAY SURVEY; FORMATION HISTORY; GOODS-HERSCHEL;

D O I：

10.1088/0004-637X/773/1/3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a measurement of the average supermassive black hole accretion rate (BHAR) as a function of the star formation rate (SFR) for galaxies in the redshift range 0.25 < z < 0.8. We study a sample of 1767 far-IR-selected star-forming galaxies in the 9 deg(2) Bootes multi-wavelength survey field. The SFR is estimated using 250 mu m observations from the Herschel Space Observatory, for which the contribution from the active galactic nucleus (AGN) is minimal. In this sample, 121 AGNs are directly identified using X-ray or mid-IR selection criteria. We combined these detected AGNs and an X-ray stacking analysis for undetected sources to study the average BHAR for all of the star-forming galaxies in our sample. We find an almost linear relation between the average BHAR (in M-circle dot yr(-1)) and the SFR (in M-circle dot yr(-1)) for galaxies across a wide SFR range 0.85 < log SFR < 2.56 : logBHAR = (-3.72 +/- 0.52) + (1.05 +/- 0.33) log SFR. This global correlation between SFR and average BHAR is consistent with a simple picture in which SFR and AGN activity are tightly linked over galaxy evolution timescales.

引用

页数：9

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