Unravelling the nature of the dual AGN in the galaxy pair system IRAS 05589+2828 and 2MASX J06021107+2828382

We have studied the nuclear region of the previously detected dual AGN system in the galaxy pair IRAS 05589+2828 and 2MASX J06021107+2828382 through new optical spectroscopy observations, along with radio and X-ray archival data. Our multiwavelength data strongly suggest that the Sy1 \iras, (z=0.0330$\pm$0.0002) conforms to a dual AGN system with the Sy2 \twomas, (z=0.0334$\pm$0.0001) with a projected separation obtained from the radio data of 20.08\arcsec, ($\sim$13.3,kpc). Analysis of the optical spectra reveals a faint narrow extended emission from H$\alpha$ and [OIII] amidst the two AGN, supporting evidence for an ongoing merger. \iras, is a double component narrow emission line AGN, with complex broad Balmer emission line profiles that clearly show a strong red-peaklet with a velocity shift of $\sim$3500,km,s${}^{-1}$. The black hole mass estimates of \iras, and \twomas, are log,M${}_{\mathrm{B}\mathrm{H}}$,=,8.59,$\pm$,0.14 (M${}_{\odot }$) and log,M${}_{\mathrm{B}\mathrm{H}}$,=,8.21$\pm$0.2 (M${}_{\odot }$), respectively. In the X-ray bands, \iras, is compatible with a Type 1 object, showing both spectral and flux variability. \chandra, data of 2MASX,J06021107+2828382 allowed us to measure a high hardness ratio in this source, providing evidence for a Type 2 AGN. The 22 GHz image obtained with the {\it Karl G. Jansky Very Large Array} has revealed that both AGN are compact radio objects with spectral indices -0.26$\pm$0.03 and -0.70$\pm$0.11, confirming for the first time its dual AGN nature in the radio bands.