A Gemini–NIFS view of the merger remnant NGC 34

• Main Author: Motter, Juliana Cristina
• Publication Date: 2021
• Other Authors: Riffel, Rogério, Ricci, Tiago Vecchi, Riffel, Rogemar André, Storchi-Bergmann, Thaisa, Pastoriza, Miriani Griselda, Rodriguez-Ardila, Alberto, Dutra, Daniel Ruschel, Hahn, Luis Gabriel Dahmer, Dametto, Natacha Zanon, Diniz, Marlon Rodrigo
• Format: Article
• Language: eng
• Source: Repositório Institucional da UFRGS
• Download full: http://hdl.handle.net/10183/235274
• topic: Galáxia NGC 34; Cinemática; Galaxias Starburst; Nucleo galatico; Galaxies : Individual : NGC 34; Galaxies : Individual : NGC 17; Galaxies : Individual : Mrk 938; Galaxies : ISM; Galaxies : Nuclei; Galaxies : Starburst; Infrared : Galaxies

The merger remnant NGC 34 is a local luminous infrared galaxy (LIRG) hosting a nuclear starburst and a hard X-ray source associated with a putative, obscured Seyfert 2 nucleus. In this work, we use adaptive optics assisted near-infrared (NIR) integral field unit observations of this galaxy to map the distribution and kinematics of the ionized and molecular gas in its inner 1.2kpc×1.2kpc⁠, with a spatial resolution of 70 pc. The molecular and ionized gas kinematics is consistent with a disc with projected major axis along a mean PA = −9∘.2 ± 0∘.9. Our main findings are that NGC 34 hosts an AGN and that the nuclear starburst is distributed in a circumnuclear star formation ring with inner and outer radii of ≈ 60 and 180 pc, respectively, as revealed by maps of the [FeII]/Paβ and H2/Br γ emission-line ratios, and corroborated by PCA tomography analysis. The spatially resolved NIR diagnostic diagram of NGC 34 also identifies a circumnuclear structure dominated by processes related to the stellar radiation field and a nuclear region where [FeII] and H2 emissions are enhanced relative to the hydrogen recombination lines. We estimate that the nuclear X-ray source can account for the central H2 enhancement and conclude that [FeII] and H2 emissions are due to a combination of photoionization by young stars, excitation by X-rays produced by the AGN and shocks. These emission lines show nuclear, broad, blueshifted components that can be interpreted as nuclear outflows driven by the AGN.