(Continued) Three-color ALMA 12 m array images of the Evolved clouds: G010.62 (panel l), W51-IRS2 (panel m), G012.80 (panel n), and G333.60 (panel o). There is an almost complete coincidence between the free-free emission at the H41α recombination line frequency (blue) and the 3 mm continuum (green), which is dominated in panels l-o by free-free emission. Red filamentary structures represent the few locations where thermal dust emission dominates the continuum millimeter emission.