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Circumnuclear star formation in Seyfert galaxies

Published online by Cambridge University Press:  07 August 2017

W. Kollatschny ,
A. Goerdt  and
K.J. Fricke
W. Kollatschny
Affiliation:
Universitäts-Sternwarte Geismarlandstr. 11 D-3400 Göttingen, F.R.G. Dr. Remeis-Sternwarte D-8600 Bamberg, F.R.G.
A. Goerdt
Affiliation:
Universitäts-Sternwarte Geismarlandstr. 11 D-3400 Göttingen, F.R.G.
K.J. Fricke
Affiliation:
Universitäts-Sternwarte Geismarlandstr. 11 D-3400 Göttingen, F.R.G.

Abstract

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Using population synthesis methods the nuclear and circumnuclear spectra of Seyfert galaxies were modeled. The central nonthermal intensity and the surrounding star formation rate are correlated.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 440
Copyright
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