The dustiest Post-Main sequence stars in the Magellanic Clouds
  Using observations from the {\em Herschel} Inventory of The Agents of Galaxy
Evolution (HERITAGE) survey of the Magellanic Clouds, we have found thirty five
evolved stars and stellar end products that are bright in the far-infrared.
These twenty eight (LMC) and seven (SMC) sources were selected from the 529
evolved star candidates in the HERITAGE far-infrared point source catalogs. Our
source identification method is based on spectral confirmation, spectral energy
distribution characteristics, careful examination of the multiwavelength images
and includes constraints on the luminosity, resulting in a thoroughly vetted
list of evolved stars. These sources span a wide range in luminosity and hence
initial mass. We found thirteen low- to intermediate mass evolved stars,
including asymptotic giant branch (AGB) stars, post-AGB stars, planetary
nebulae and a symbiotic star. We also identify ten high mass stars, including
four of the fifteen known B[e] stars in the Magellanic Clouds, three extreme
red supergiants which are highly enshrouded by dust, a Luminous Blue Variable,
a Wolf-Rayet star and two supernova remnants. Further, we report the detection
of nine probable evolved objects which were previously undescribed in the
literature. These sources are likely to be among the dustiest evolved objects
in the Magellanic Clouds. The {\em Herschel} emission may either be due to dust
produced by the evolved star or it may arise from swept-up ISM material.
