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

Gaseous Material Orbiting the Polluted, Dusty White Dwarf HE1349-2305