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1.8. Evolutionary population synthesis of AGN host galaxy spectra

Published online by Cambridge University Press:  25 May 2016

W. Kollatschny  and
A. Goerdt
W. Kollatschny
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
A. Goerdt
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany

Abstract

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We compute the stellar population of nearby Seyfert host galaxies and non-active galaxies using population and evolutionary synthesis methods. We find indication of enhanced star formation rates in the host-galaxies of AGN - especially in the circumnuclear regions of Seyfert 2 galaxies.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 31 - 32
Copyright
Copyright © Kluwer 1998 

References

Bertelli, G., et al., (1994) ApjS 106, 275.Google Scholar
Goerdt, A., Fricke, K.J., Kollatschny, W., (1993) ApSS 205, 5.Google Scholar
Goerdt, A., Kollatschny, W. (1996), Proc. of Conf. on “From Stars to Galaxies: The impact of Stellar Physics on Galaxy Evolution”, Crete, Ed.: Leitherer, et al., ASP Conf. Ser.98, 521.Google Scholar
Kollatschny, W., Goerdt, A. (1997), ESO Symp. on “The Early Universe with the VLT”, Ed.:Bergeron, , 400.Google Scholar
Pickles, A.J., van der Kruit, P.C., (1990) A&AS 84, 421.Google Scholar