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Radiative shock models for the NLR of AGN: Predictions up to 1000 km s−1

Published online by Cambridge University Press:  24 November 2004

M. G. Allen ,
R. Sutherland ,
M. A. Dopita ,
L. J. Kewley  and
B. A. Groves
M. G. Allen
Affiliation:
Observatoire de Strasbourg UMR 7550, Strasbourg, France email:allen@newb6.u-strasbg.fr
R. Sutherland
Affiliation:
RSAA, Australian National University, Australia
M. A. Dopita
Affiliation:
RSAA, Australian National University, Australia
L. J. Kewley
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, USA
B. A. Groves
Affiliation:
RSAA, Australian National University, Australia
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Abstract

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High velocity shocks may provide an important source of ionizing radiation in the NLR of active galaxies. Here we present preliminary results of a new grid of MAPPINGS III shock models for shock velocities up to 1000 km s−1. This grid significantly extends the parameter space covered by the previous models, and will serve as an important component in building multi-process models of the NLR.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 305 - 306
Copyright
© 2004 International Astronomical Union