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2.5–11.6 μ Spectrophotometry and Imaging of AGNs

Published online by Cambridge University Press:  25 May 2016

J. Clavel ,
B. Schulz ,
B. Altieri ,
P. Barr ,
P. Claes ,
A. Heras ,
K. Leech ,
L. Metcalfe  and
A. Salama
J. Clavel
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
B. Schulz
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
B. Altieri
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
P. Barr
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
P. Claes
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
A. Heras
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
K. Leech
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
L. Metcalfe
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain
A. Salama
Affiliation:
ISO Science Operations Centre, Astrophysics Division, ESA Space Science Dept.,P.O. Box 50727, 28080 Madrid, Spain

Abstract

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We present low resolution spectrophotometric and imaging ISO observations of a sample of 58 AGN's over the 2.5–11.6 μ range. The data strongly support unification schemes and set new constraints on models of the molecular torus.

Type
II. Observational Properties of AGN and Related Objects
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 145 - 150
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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