# A Near Infrared View of Nearby Galaxies: The Case of NGC 6300

## TL;DR

This study uses near-infrared imaging and spectroscopy to analyze the nuclear structure, gas dynamics, and dust properties of the Seyfert 2 galaxy NGC 6300, revealing off-center black hole activity and nuclear obscuration mechanisms.

## Contribution

It provides high-resolution near-infrared observations of NGC 6300, estimating black hole mass, detecting nuclear outflows, and characterizing dust distribution and obscuration beyond the classical torus.

## Key findings

- Black hole is offset by 25 pc from galaxy center.
- Estimated black hole mass is approximately 6 x 10^7 solar masses.
- Detected nuclear outflow via asymmetric Paβ emission.

## Abstract

We present a near-infrared study of the Seyfert 2 galaxy NGC\,6300, based on subarcsecond images and long slit spectroscopy obtained with Flamingos-2 at Gemini South. We have found that the peak of the nuclear continuum emission in the $K_s$ band and the surrounding nuclear disk are 25\,pc off-center with respect to the center of symmetry of the larger scale circumnuclear disk, suggesting that this black hole is still not fixed in the galaxy potential well. The molecular gas radial velocity curve yields a central black hole upper mass estimation of $M_{SMBH}^{upper}=(6\pm 2) \times 10^{7}\,\Msun$. The Pa$\beta$ emission line has a strongly asymmetric profile with a blueshifted broad component that we associate with a nuclear ionized gas outflow. We have found in the $K_s$-band spectra that the slope of the continuum becomes steeper with increasing radii, which can be explained as the presence of large amounts of hot dust not only in the nucleus but also in the circumnuclear region up to $r=27$\,pc. In fact, the nuclear red excess obtained after subtracting the stellar contribution resembles to that of a blackbody with temperatures around 1200\,K. This evidence supports the idea that absorbing material located around the nucleus, but not close enough to be the torus of the unified model, could be responsible for at least part of the nuclear obscuration in this Seyfert 2 nucleus.