Aromatic features in AGNs: star-forming infrared luminosity function of AGN host galaxies

被引：0

作者：

Shi, Yong ^{[1
]}

Ogle, Patrick ^{[2
]}

Rieke, George H. ^{[1
]}

Antonucci, Robert ^{[3
]}

Hines, Dean C. ^{[4
]}

Smith, Paul S. ^{[1
]}

Low, Frank J. ^{[1
]}

Bouwman, Jeroen ^{[5
]}

Willmer, Christopher ^{[1
]}

机构：

[1] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[2] CALTECH, Spire Sci Ctr, Pasadena, CA 91125 USA

[3] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[4] Space Sci Inst, Boulder, CO 80301 USA

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

来源：

STARBURST-AGN CONNECTION | 2009年 / 408卷

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

EMISSION FEATURES; SPECTRA; NUCLEI; SEARCH;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe observations of aromatic features at 7.7 and 11.3 mu m in AGNs of three types including PG, 2MASS and 3CR objects. The features have been demonstrated to originate predominantly from star formation. The star-forming infrared luminosity function of PG quasars is flatter than that of field galaxies, implying nuclear activity and star formation tend to be enhanced together. A high detection rate of aromatic features in a complete z similar to 1 quasar sample implies a stronger evolution of star formation in quasar hosts than that in field galaxies.

引用

页码：209 / +

页数：3

共 18 条

[1]

Cutri RM, 2001, ASTR SOC P, V232, P78

[2] The infrared spectral energy distribution of normal star-forming galaxies: Calibration at far-infrared and submillimeter wavelengths [J].

Dale, DA ;

Helou, G .

ASTROPHYSICAL JOURNAL, 2002, 576 (01) :159-168

[3]

DESERT FX, 1988, ASTRON ASTROPHYS, V206, P227

[4] [O II] emission in quasar host galaxies: Evidence for a suppressed star formation efficiency [J].

Ho, LC .

ASTROPHYSICAL JOURNAL, 2005, 629 (02) :680-685

[5] INWARD BOUND - THE SEARCH FOR SUPERMASSIVE BLACK-HOLES IN GALACTIC NUCLEI [J].

KORMENDY, J ;

RICHSTONE, D .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1995, 33 :581-624

[6]

Laurent O, 2000, ASTRON ASTROPHYS, V359, P887

[7] Infrared luminosity functions from the Chandra Deep Field-South:: The Spitzer view on the history of dusty star formation at 0 ≤ z ≤ 1 [J].

Le Floc'h, E ;

Papovich, C ;

Dole, H ;

Bell, EF ;

Lagache, G ;

Rieke, GH ;

Egami, E ;

Pérez-González, PG ;

Alonso-Herrero, A ;

Rieke, MJ ;

Blaylock, M ;

Engelbracht, CW ;

Gordon, KD ;

Hines, DC ;

Misselt, KA ;

Morrison, JE ;

Mould, J .

ASTROPHYSICAL JOURNAL, 2005, 632 (01) :169-190

[8] Infrared emission of normal galaxies from 2.5 to 12 micron:: Infrared Space Observatory spectra, near-infrared continuum, and mid-infrared emission features [J].

Lu, NY ;

Helou, G ;

Werner, MW ;

Dinerstein, HL ;

Dale, DA ;

Silbermann, NA ;

Malhotra, S ;

Beichman, CA ;

Jarrett, TH .

ASTROPHYSICAL JOURNAL, 2003, 588 (01) :199-217

[9] The demography of massive dark objects in galaxy centers [J].

Magorrian, J ;

Tremaine, S ;

Richstone, D ;

Bender, R ;

Bower, G ;

Dressler, A ;

Faber, SM ;

Gebhardt, K ;

Green, R ;

Grillmair, C ;

Kormendy, J ;

Lauer, T .

ASTRONOMICAL JOURNAL, 1998, 115 (06) :2285-2305

[10] NEW CONSTRAINTS ON THE UNIFIED MODEL OF SEYFERT-GALAXIES [J].

MAIOLINO, R ;

RUIZ, M ;

RIEKE, GH ;

KELLER, LD .

ASTROPHYSICAL JOURNAL, 1995, 446 (02) :561-573

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