Circumnuclear populations in nearby AGN

Details Circumnuclear populations in nearby AGN Circumnuclear populations in nearby AGN

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205....5g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 5-12.

Astronomy and Astrophysics

Astrophysics

4

Active Galactic Nuclei, Seyfert Galaxies, Star Distribution, Star Formation, B Stars, Nonthermal Radiation, O Stars

Scientific paper

Using population synthesis methods we determined the relative stellar components around Seyfert nuclei in their host galaxies and the nonthermal flux contribution from the nuclei. Knowing the stellar components from the spatially resolved spectra of our objects, we can calculate the number of OB-stars and from that the star formation rate. We found that the contribution of OB-stars is correlated with the strength of the nonthermal flux at the nucleus.

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