  The empirical evidence for an upper mass limit for the red supergiant (RSG)
progenitors of the Type II-P SNe at about 18 Msun, raises questions about the
fate of the most luminous, most massive RSGs. These stars may evolve back to
warmer temperatures to end their lives as hotter stars or collapse directly to
black holes. The yellow hypergiants, many with extensive circumstellar dust and
high mass loss, are excellent candidates for post-RSG evolution. We have
identified six high luminosity yellow supergiants (YSGs) in the LMC with
circumstellar dust including two of the FYPS (Dorn et al, 2022). We discuss
their SEDs, mass lost and mass loss rates. Together with three additional FYPS,
these nine stars are about 1/3 of the YSGs above 10^5 Lsun. We conclude that
the high luminosity YSGs with surface pulsations and circumstellar dust,
distinct from other YSGs, are candidates for post-RSG evolution in the LMC.
