Emitting gas regions in Mrk 493: An extensive Fe II line emission region

Details Emitting gas regions in Mrk 493: An extensive Fe II line emission region Emitting gas regions in Mrk 493: An extensive Fe II line emission region

2007-01-24

arxiv.org/abs/astro-ph/0701684v1

Astronomy and Astrophysics

Astrophysics

To appear in the Proceedings of "The Central Engine of Active Galactic Nuclei", editors L. C. Ho and J.-M. Wang

Scientific paper

We performed 3D spectroscopic observations of Mrk 493 in order to investigate
the Fe II emitting region and their possible connection with the Hydrogen
emitting region. We found that there is a strong Fe II emission in an extensive
region ~ 4" x 4" around Sy 1 nucleus. The Fe II line width indicates that these
lines are originated in an intermediate line region.

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