Detection of a Triple Nucleus in the Wolf–Rayet Composite Sy 2 Galaxy NGC 6764

Abstract

We report adaptive-optics Ks-band imaging of the composite Seyfert 2 and Wolf–Rayet galaxy NGC 6764 (D = 32 Mpc), obtained with LUCI/SOUL at the Large Binocular Telescope (LBT). The nucleus resolves into three compact sources with pairwise projected separations of 0.″07 – 0.″2 , corresponding to 11.0–30.9 pc. All three have indistinguishable H, Ks, H2, and Brγ colors, so photometry alone cannot separate accretion from star formation. The system is consistent with a Seyfert nucleus and two star-forming regions, but a dual or triple active galactic nucleus (AGN) cannot be excluded. In case of the latter, the separations would be two orders of magnitude smaller than in any confirmed or candidate AGN triplet reported to date. Diffraction-limited near-infrared integral-field spectroscopy is required to establish the nature of each component.