NGC 985 - Interactions and the origin of AGNs

Details NGC 985 - Interactions and the origin of AGNs NGC 985 - Interactions and the origin of AGNs

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171..131r&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Emission Spectra, Far Infrared Radiation, Galactic Structure, Seyfert Galaxies, Stellar Luminosity, Astronomical Spectroscopy, H Ii Regions, H Lines, Infrared Astronomy Satellite, Lyman Spectra, Star Formation

Scientific paper

Observations of the Seyfert galaxy NGC 985 have revealed large-scale
extended ionized zones, covering a large fraction of the ring-shaped
structure of this galaxy. These ionized regions are a major contributor
to the total far-infrared emission of this object. An interaction driven
starburst is proposed to explain the main features of this galaxy.

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