LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$

TL;DR

This study uses high-resolution imaging and radio observations to analyze galaxy structures and their relation to nuclear activity, revealing that bulge properties strongly correlate with radio emission across diverse galaxy types.

Contribution

It provides a detailed multi-component decomposition of galaxy structures, highlighting the importance of including various components for accurate bulge mass estimation and its relation to nuclear radio activity.

Findings

Bulge mass overestimation occurs when non-bulge components are ignored.

Bulges grow larger and more prominent from irregular to elliptical galaxies.

Radio detection fraction increases with bulge mass, reaching 77% for M_bulge > 10^11 M_sun.

Abstract

[Abridged] We use high-resolution $HST$ imaging and $e$-MERLIN 1.5-GHz observations of galaxy cores from the LeMMINGs survey to investigate the relation between optical structural properties and nuclear radio emission for a large sample of galaxies. We perform accurate, multi-component decompositions of new surface brightness profiles extracted from $HST$ images for 163 LeMMINGs galaxies and fit up to six galaxy components (e.g., bulges, discs, AGN, bars, rings, spiral arms, and nuclear star clusters) simultaneously with S\'ersic and/or core-S\'ersic models. By adding such decomposition data for 10 LeMMINGs galaxies from our past work, the final sample of 173 nearby galaxies (102 Ss, 42 S0s, 23 Es plus 6 Irr) with bulge stellar mass (typically) M_*, bulge ~ 10^6-10^12.5 M_sun, encompasses all optical spectral classes (LINER, Seyfert, ALG and H II). We show that the bulge mass can be significantly overestimated in many galaxies when components such as bars, rings and spirals are not included in the fits. We additionally implement a Monte Carlo method to determine errors on bulge, disc and other fitted structural parameters. Moving (in the opposite direction) across the Hubble sequence, i.e., from the irregular to elliptical galaxies, we confirm that bulges become larger, more prominent and round. Such bulge dominance is associated with a brighter radio core luminosity. We also find that the radio detection fraction increases with bulge mass. At M_*,bulge > 10^11 M_sun, the radio detection fraction is 77%, declining to 24% for M_bulge < 10^10 M_sun. Furthermore, we observe core-S\'ersic bulges tend to be systematically round and to possess high radio core luminosities and boxy-distorted or pure elliptical isophotes.