Emitting gas regions in Mrk 493: An extensive Fe II line emission region
classification
🌌 astro-ph
keywords
regionemittinglineemissionextensivearoundconnectionfound
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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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