  We present new spectroscopic observations of the polluted, dusty,
helium-dominated atmosphere white dwarf star HE1349-2305. Optical spectroscopy
reveals weak CaII infrared triplet emission indicating that metallic gas debris
orbits and is accreted by the white dwarf. Atmospheric abundances are measured
for magnesium and silicon while upper limits for iron and oxygen are derived
from the available optical spectroscopy. HE1349-2305 is the first gas
disk-hosting white dwarf star identified amongst previously known polluted
white dwarfs. Further characterization of the parent body polluting this star
will require ultraviolet spectroscopy.
