An interacting galaxy pair at the origin of a light echo
Paola Merluzzi, Giovanni Busarello, Michael A. Dopita, Adam D. Thomas,, Chris P. Haines, Aniello Grado, Luca Limatola, Amata Mercurio

TL;DR
This study presents the first observed case of a light echo between two galaxies, revealing a fading AGN that previously ionized a large region in a companion galaxy, supported by detailed multi-wavelength observations and modeling.
Contribution
It provides the first direct evidence of a light echo between galaxies, combining integral-field spectroscopy and multi-band data to analyze AGN fading and galaxy interaction.
Findings
Detected a 2-3 kpc AGN outflow and hollow bicone structure.
Confirmed a first encounter between the galaxies at 21 kpc apart.
Found the AGN luminosity to be 20 times lower than needed to excite the EELR.
Abstract
In a low-density region of the Shapley supercluster we identified an interacting galaxy pair at redshift z=0.04865 in which the Seyfert-2 nucleus of the main galaxy (ShaSS 073) is exciting an extended emission line region (EELR, ~170 kpc^2) in the disk of the less massive companion (ShaSS 622). New integral-field spectroscopy and the multi-band data-set, spanning from far-ultraviolet to far-infrared and radio wavelengths, allowed us to obtain a detailed description of the ShaSS 622-073 system. The gas kinematics shows hints of interaction, although the overall velocity field shows a quite regular rotation in both galaxies, thus suggesting that we are observing their first encounter as confirmed by the estimated distance of 21 kpc between the two galaxy centers. The detected ~2-3 kpc AGN outflow and the geometry of the EELR in ShaSS 622 support the presence of a hollow bicone structure.…
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