MIR AND HARD X-RAY LUMINOSITIES, SILICATE FEATURES, AND SFR IN AGN

被引：0

作者：

Juarez, Y. ^{[1
]}

Maiolino, R. ^{[2
]}

Mujica, R. ^{[1
]}

Cruz-Gonzalez, I. ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City 04510, DF, Mexico

[2] INAF Osservatorio Astron Roma, I-00040 Monte Porzio Catone, Italy

来源：

XIII LATIN AMERICAN REGIONAL IAU MEETING | 2011年 / 40卷

关键词：

ULTRALUMINOUS INFRARED GALAXIES; SPECTRAL ENERGY-DISTRIBUTIONS; QSOS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate the obscuration and star formation activity in local AGN by exploiting a large compilation of Spitzer-IRS spectra. In order to avoid biases due to the obscuration itself and to measure the intrinsic luminosity in a homogeneous manner in both, obscured and unobscured objects, we have selected a sample of local AGN observed with Spitzer-IRS having hard X-ray spectra. The analysis of a large sample allows us to investigate the relationship between obscuration, dust covering factor, star formation rate (SFR) and intrinsic luminosity of the AGN.

引用

页码：124 / 124

页数：1

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