Double-nucleus elliptical MCG-01-12-005 in an X-ray emitting cluster of galaxies
Roberto Nesci (1), Mariateresa Fiocchi (1), Loredana Bassani (2),, Pietro Parisi (1) ((1) INAF/IAPS, (2) INAF/IASFBO)

TL;DR
This paper reports the discovery of a double-nucleus elliptical galaxy within an X-ray emitting cluster, providing evidence of a galaxy merger in progress, supported by photometric and spectroscopic analysis.
Contribution
It presents a detailed observational case of a merging elliptical galaxy with two nuclei, confirmed by consistent redshifts and spectral features, adding to understanding of galaxy formation processes.
Findings
Two nuclei have similar colors and spectra, indicating a merger.
Redshifts of both nuclei match, confirming they are part of the same galaxy.
The galaxy is located in an X-ray emitting cluster, supporting the merger scenario.
Abstract
The scenario of galaxy formation is believed to follow a structure that builds up from the bottom, with large galaxies being formed by several merging episodes of smaller ones. In this scenario a number of galaxies can be expected to be seen in the merging phase, with their external regions already mixed, while their nuclei, with stronger self-gravitation, are still recognizable as such. During a photometric monitoring of AGNs in the field of a long-exposure INTEGRAL pointing, we serendipitously found an elliptical galaxy in the center of the X-ray cluster (EXO 0422-086) with two nuclei. We performed surface photometry on our images and those of the SDSS archive and obtained slit spectra of both nuclei. Aperture photometry of the two stellar-like nuclei showed very similar colors in the SDSS image and in our Johnson BVRI images, which is typical of an elliptical galaxy nucleus. The…
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