ISOCAM-CVF 5-12 micron spectroscopy of ultraluminous infrared galaxies

被引:194
作者
Tran, QD
Lutz, D
Genzel, R
Rigopoulou, D
Spoon, HWW
Sturm, E
Gerin, M
Hines, DC
Moorwood, AFM
Sanders, DB
Scoville, N
Taniguchi, Y
Ward, M
机构
[1] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[2] European So Observ, D-85748 Garching, Germany
[3] Ecole Normale Super Radioastron, F-75231 Paris, France
[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[5] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[6] CALTECH, Pasadena, CA 91125 USA
[7] Tohoku Univ, Inst Astron, Aoba Ku, Sendai, Miyagi 9808758, Japan
[8] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
关键词
galaxies : active; galaxies : starburst; infrared : galaxies;
D O I
10.1086/320543
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present low-resolution mid-infrared (MIR) spectra of 16 ultraluminous infrared galaxies (ULIRGs) obtained with the circular variable filter (CVF) spectroscopy mode of ISOCAM on board the Infrared Space Observatory (ISO). Our sample completes previous ISO spectroscopy of ultra- and hyperluminous infrared galaxies toward higher luminosities. The combined samples cover an infrared luminosity range of similar to 10(12)-10(13.1) L.. To discriminate active galactic nucleus (AGN) and starburst activity, we use the AGN-related MIR continuum and the starburst-related 6.2, 7.7, 8.6, and 11.3 mum MIR emission bands attributed to aromatic carbonaceous material. For about half of the high-luminosity ULIRGs studied here, strong aromatic emission bands suggest starburst dominance. Other spectra are dominated by a strong AGN-related continuum with weak superposed emission features of uncertain nature. Our sample contains one unusual example, IRAS F00183-7111, of an AGN that is highly obscured even in the MIR. An improved method to characterize quantitatively the relative contribution of star formation and AGN activity to the MIR emission of ULIRGs is presented. The ULIRG spectra are fitted by a superposition of a starburst and an AGN spectrum, both of which may be obscured at different levels. Models in which starburst and AGN obscuration differ are significantly more successful than models with a single extinction. Previous results based on a simpler line-to-continuum measure of aromatic emission strength are confirmed, further supporting the robustness of the aromatic emission feature as a diagnostic of ULIRG power sources. As dominant sources of the bolometric luminosity, starbursts prevail at the lower end and AGNs at the higher end of this range. The transition between mostly starburst and mostly AGN powered occurs at similar to 10(12.4)-10(12.5) L., and individual luminous starbursts are found up to,similar to 10(12.65) L..
引用
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页码:527 / 543
页数:17
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