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Probing the heart of an active galactic nucleus: NGC 1068

Abstract:
We present results from integral field spectroscopy of the narrow line region of NGC 1068, carried out with the MPE 3D near infrared imaging spectrometer. A map and velocity field of the [Fe II] fine structure line at 1.64mum is presented. The kinematics of the [Fe II] emission, which arises in partially ionized zones, shows red shifted emission in the north eastern cone of the NLR, and blue shifted emission in the south west, reversed relative to high ionization species such as [Si VI] or [0 111]. We propose a model geometry of the narrow line region which is consistent with existing data and explains the observed [Fe II] kinematics.
Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
GALAXIES AND THEIR CONSTITUENTS AT THE HIGHEST ANGULAR RESOLUTIONS More from this journal
Issue:
205
Pages:
216-219
Publication date:
2001-01-01
Event title:
24th General Assembly of the International-Astronomical-Union
ISSN:
0074-1809
ISBN:
1583810668


Keywords:
Pubs id:
pubs:22528
UUID:
uuid:016ff78e-6f43-4536-980c-71cd92680a33
Local pid:
pubs:22528
Source identifiers:
22528
Deposit date:
2012-12-19
ARK identifier:

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