A resolved study of the inner regions of nearby galaxies with an excess of young massive stars: missing link in the AGN-starburst connection?

Abstract

We have selected galaxies with very high levels of H$\hat{I}\pm$ emission (EQW(H$\hat{I}\pm$)$>$700 Ã .) in their central regions from the final data release of the MaNGA survey . Our study focuses on 14 very well-resolved nearby galaxies with stellar masses in the range $9.5<\log M_{\ast }/(M_{\odot })<11.5$. We investigate a variety of procedures for selecting galaxy regions that are likely to harbour excess populations of young massive stars, finding that selection in the 2-dimensional space of extinction-corrected H$\hat{I}\pm$ EQW and [SIII]/[SII] line ratio produces the best results. By comparing stacked spectra covering these regions with stacked spectra covering normal starburst regions with 100Ã $<$EQW(H$\hat{I}\pm$)$<$200Ã , we obtain the following main results: 1) Clear signatures of excess Wolf Rayet stars are found in half of the H$\hat{I}\pm$ excess regions, 2) Galaxy regions containing excess Wolf Rayet stars are more often associated with the presence of high-ionization emission lines characteristic of accreting black holes. Excess [NeIII] is detected in 4 out of 8 of the WR regions and there are tentative [FeX] detections in 2 galaxies. 3) Regions of the galaxy with excess Wolf Rayet stars are located where the interstellar medium has larger ionized gas turbulent velocities and higher neutral gas overdensities. We make a first attempt to constrain changes in the high mass end of the stellar initial mass function (IMF) using the HR-pyPopStar evolutionary population synthesis models that include high wavelength-resolution theoretical atmosphere libraries for Wolf Rayet stars.

accepted for publication in MNRAS