PAH emission and star formation in the host of the z∼2.56 Cloverleaf QSO

被引:47
作者
Lutz, D. [1 ]
Sturm, E.
Tacconi, L. J.
Valiante, E.
Schweitzer, M.
Netzer, H.
Maiolino, R.
Andreani, P.
Shemmer, O.
Veilleux, S.
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[2] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[3] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Wise Observ, IL-69978 Tel Aviv, Israel
[4] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
[5] ESO, D-85748 Garching, Germany
[6] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[7] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
关键词
galaxies : active; galaxies : starburst; infrared : galaxies;
D O I
10.1086/518537
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the first detection of the 6.2 and 7.7 mu m infrared polycyclic aromatic hydrocarbon ( PAH) emission features in the spectrum of a high-redshift QSO, from the Spitzer IRS spectrum of the Cloverleaf lensed QSO ( H1413 + 117, z similar to 2.56). The ratio of PAH features and rest-frame far-infrared emission is the same as in lower luminosity star-forming ULIRGs and in local PG QSOs, supporting a predominantly starburst nature of the Cloverleaf's huge far-infrared luminosity (5.4 x 10(12) L-circle dot, corrected for lensing). The Cloverleaf's period of dominant QSO activity (L-Bol similar to 7 x 10(13) L-circle dot) is coincident with an intense (star formation rate similar to 1000 M-circle dot yr(-1)) and short (gas exhaustion time similar to 3 x 10(7) yr) star-forming event.
引用
收藏
页码:L25 / L28
页数:4
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