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It is imperative to map the strength and distribution of feedback in galaxiesto understand how feedback affects the galactic ecosystems. H$_2$O masers actas indicators of energy injection into the ISM. Our goal is to measure thestrength and distribution of feedback traced by water masers in the Milky Way.We identify optical counterparts to H$_2$O masers discovered by the HOPSsurvey. The distribution and luminosities of H$_2$O masers in the Milky Way aredetermined using parallax measurements derived from the second Gaia DataRelease. We provide evidence of a correlation between evolved stars, as tracedby H$_2$O masers, and the spiral structure of the Milky Way, suggesting a linkbetween evolved stars and the Galactic environment.

Evidence for Coupling of Evolved Star Atmospheres and Spiral Arms of the Milky Way