THE DIFFERENCES IN THE TORUS GEOMETRY BETWEEN HIDDEN AND NON-HIDDEN BROAD LINE ACTIVE GALACTIC NUCLEI

Ichikawa, Kohei; Packham, C.; Ramos Almeida, C.; Asensio Ramos, A.; Alonso‐Herrero, A.; González-Martín, O.; López-Rodríguez, Enrique; Ueda, Yoshihiro; Díaz-Santos, T.; Elitzur, Moshe; F. Hönig, S.; Imanishi, Masatoshi; A. Levenson, N.; Mason, Rachel; S. Perlman, Eric; D. Alsip, Crystal

doi:10.1088/0004-637x/803/2/57

Public

THE DIFFERENCES IN THE TORUS GEOMETRY BETWEEN HIDDEN AND NON-HIDDEN BROAD LINE ACTIVE GALACTIC NUCLEI

Shared by NobleBlocks on Apr 15, 2015 • 12:00 AM UTC

Authors:

Kohei Ichikawa

C. Packham

C. Ramos Almeida

Abstract

We present results from the fitting of infrared (IR) spectral energy distributions of 21 active galactic nuclei (AGNs) with clumpy torus models. We compiled high spatial resolution (0.3-0.7 arcsec) mid-IR (MIR) N-band spectroscopy, Q-band imaging, and nuclear near-and MIR photometry from the literat...

Subject

Torus

Physics

Astrophysics

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