Mid-infrared spectroscopy of high-redshift submillimeter galaxies:: First results

被引:83
作者
Menendez-Delmestre, Karin [1 ]
Blain, Andrew W.
Alexander, Dave M.
Smail, Ian
Armus, Lee
Chapman, Scott C.
Frayer, D. T.
Ivison, Rob J.
Teplitz, H. I.
机构
[1] CALTECH, Pasadena, CA 91125 USA
[2] Univ Durham, Inst Computat Cosmol, Durham DH1 3HP, England
[3] CALTECH, Spitzer Sci Ctr, Pasadena, CA USA
[4] Astron Inst, Cambridge, England
[5] UK Astron Technol Ctr, Edinburgh, Midlothian, Scotland
[6] Inst Astron, Edinburgh, Midlothian, Scotland
基金
英国科学技术设施理事会;
关键词
galaxies : active; galaxies : starburst; infrared : galaxies; techniques : spectroscopic; ULTRALUMINOUS INFRARED GALAXIES; SPITZER-SPACE-TELESCOPE; SCUBA SUPER-MAP; LENSING CLUSTERS; SPECTROGRAPH IRS; NUMBER COUNTS; SPECTRA; FIELD; EVOLUTION; FEATURES;
D O I
10.1086/512038
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present mid-infrared spectra of five submillimeter galaxies at taken with the Spitzer Space z p 0.65-2.38 Telescope. Four of these sources, at, have strong PAH features and their composite spectrum is well z <= 1.5 fitted by an M82-like spectrum with an additional power-law component consistent with that expected from AGN activity. Based on comparison with local templates of the 7.7 mu m PAH equivalent width and the PAH-to-infrared luminosity ratio, we conclude that these galaxies host both star formation and AGN activity, with star formation dominating the bolometric luminosity. The source at displays a Mrk 231-type broad emission feature z = 2.38 at rest frame similar to 8 mm that does not conform to the typical 7.7 mu m/8.6 mm PAH complex in starburst galaxies, suggesting a more substantial AGN contribution.
引用
收藏
页码:L65 / L68
页数:4
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