Star formation and AGN

Details Star formation and AGN Star formation and AGN

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..127g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 127-134.

Astronomy and Astrophysics

Astrophysics

13

Active Galactic Nuclei, H Alpha Line, Spiral Galaxies, Star Formation, Emission Spectra, Nonthermal Radiation, Oxygen Spectra

Scientific paper

We analyze the data from narrow band H-alpha and forbidden O III CCD imaging of a sample of nearby spiral galaxies with active nuclei. The results show that the large scale star formation depends on the level of nuclear activity, with Seyfert 2 presenting the strongest disk and circumnuclear star formation, while Seyfert 1 shows very little. We present particular results for the galaxies NGC 3982, NGC 4579, NGC 5427, and NGC 7469.

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