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

L. C. Popovic·A. Smirnova·D. Ilic·A. Moiseev·J. Kovacevic·V. Afanasiev
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Abstract

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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L. C. Popovic, A. Smirnova, D. Ilic, A. Moiseev, J. Kovacevic, V. Afanasiev. 2007-01-24. Emitting gas regions in Mrk 493: An extensive Fe II line emission region. https://arxiv.org/abs/astro-ph/0701684

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