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Transition (LINER/HII) nuclei as evolved Composite (Seyfert 2/Starburst) nuclei

Published online by Cambridge University Press:  01 December 2004

Thaisa Storchi-Bergmann ,
C. H. Brandt ,
R. Cid Fernandes ,
H. R. Schmitt  and
R. González Delgado
Thaisa Storchi-Bergmann
Affiliation:
Instituto de Física, UFRGS, Porto Alegre, RS, Brazil e-mail: thaisa@if.ufrgs.br
C. H. Brandt
Affiliation:
Instituto de Física, UFRGS, Porto Alegre, RS, Brazil e-mail: thaisa@if.ufrgs.br
R. Cid Fernandes
Affiliation:
Departamento de Física, CFM – UFSC, Florianópolis, SC, Brazil e-mail: cid@astro.fs.ufsc.br
H. R. Schmitt
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA22903, USA
R. González Delgado
Affiliation:
Instituto de Astrofísica de Andalucía (CSIC), Granada 18080, Spain e-mail: rosa@iaa.es
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Abstract

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We compare the circumnuclear stellar population and environmental properies of Seyfert and Composite (Seyfert + Starburst) nuclei with those of LINERs and LINER/HII transition galaxies (TOs), and discuss evidence for evolution from Seyfert/Composite to LINER/TO nuclei.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 467 - 468
Copyright
© 2004 International Astronomical Union