******************************************************
   PR # 41105
   Warm ultraluminous infrared galaxies have L_FIR >10E12Lo and rather
   warm infrared spectra (25-60micron). Their number density in the
   local universe is comparable with that of cold ultraluminous galaxies
   and of quasars, so there must be an evolutional connection between
   them and the warm ones are considered to be in the intermediate
   states. We propose the observations of two warm ultraluminous
   galaxies in order to determine the quantity of the dust surrounding
   the central nucleus and to reveal the connection between
   ultraluminous galaxies ane quasars.
  ******************************************************