Volume 331 - Frontier Research in Astrophysics – III (FRAPWS2018) - Cosmology
A possible binary nuclei in Mrk 622
J.M. Rodriguez Espinosa*, E. Benitez, I. Cruz-González, O.G. Martín, A. Negrete, D. Ruschel-Dutra, L. Gutierrez and E. Jimenez-Bailon
*: corresponding author
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Pre-published on: October 09, 2018
Published on: November 20, 2019
Abstract
We have performed optical spectroscopy of Mrk 622 finding that it shows tripled peaked features. These features are separated in velocity showing two components that are blue-shifted and re- shifted with respect to the systemic velocity, and a third component that is right at the systemic velocity. Besides, when analysing their spectra we find that the ratio of the [OIII] to Hβ and [NII] to Hα lay in the locus of AGN for the blue and red-shifted components, while the systemic velocity component lays at the starburst/HII locus. This is interpreted as having a binary AGN that is orbiting a central Starburst.
DOI: https://doi.org/10.22323/1.331.0028
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