  We have selected galaxies with very high levels of H$\alpha$ emission
(EQW(H$\alpha$)$>$700 \AA.) 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 $9.5 < \log M_*/(M_{\odot}) < 11.5$.
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$\alpha$ 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 100\AA$<$EQW(H$\alpha$)$<$200\AA, we obtain the following main results: 1)
Clear signatures of excess Wolf Rayet stars are found in half of the H$\alpha$
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.
