We report the detection of the heavy elements Ca, Mg, Fe in the atmosp
here of the variable DA white dwarf G29-38. The abundance of Ca can be
understood only if accretion from interstellar matter is going on cur
rently at a high rate. This lends support also to the interpretation o
f the observed infrared excess as due to heated circumstellar material
, from which the accretion onto the star takes place.