# MUSE-AO view of the starburst-AGN connection: NGC 7130

## TL;DR

This study uses high-resolution adaptive optics integral field spectroscopy to reveal a decoupled core, star-forming ring, and AGN-driven outflow in NGC 7130, providing detailed insights into the starburst-AGN connection.

## Contribution

First high-resolution AO-assisted integral field observations of NGC 7130 uncover a decoupled core, star-forming ring, and AGN outflow, advancing understanding of galaxy nucleus dynamics.

## Key findings

- Detection of a 60 pc decoupled core.
- Identification of an AGN-driven outflow jet.
- Observation of a star-forming ring at 185 pc radius.

## Abstract

We present the discovery of a small kinematically decoupled core of 0.2$^{\prime\prime}$ (60 pc) in radius as well as an outflow jet in the archetypical AGN-starburst "composite" galaxy NGC 7130 from integral field data obtained with the adaptive optics-assisted MUSE-NFM instrument on the VLT. Correcting the already good natural seeing at the time of our science verification observations with the four-laser GALACSI AO system, we reach an unprecedented spatial resolution at optical wavelengths of around 0.15$^{\prime\prime}$. We confirm the existence of star-forming knots arranged in a ring of 0.58$^{\prime\prime}$ (185 pc) in radius around the nucleus, previously observed from UV and optical Hubble Space Telescope and CO(6-5) ALMA imaging. We determine the position of the nucleus as the location of a peak in gas velocity dispersion. A plume of material extends towards the NE from the nucleus until at least the edge of our field of view at 2$^{\prime\prime}$ (640 pc) radius which we interpret as an outflow jet originating in the AGN. The plume is not visible morphologically, but is clearly characterised in our data by emission-line ratios characteristic of AGN emission, enhanced gas velocity dispersion, and distinct non-circular gas velocities. Its orientation is roughly perpendicular to the line of nodes of the rotating host galaxy disc. A circumnuclear area of positive and negative velocities of 0.2$^{\prime\prime}$ in radius indicates a tiny inner disc, which can only be seen after combining the integral field spectroscopic capabilities of MUSE with adaptive optics.