A spectroscopic survey of unstudied Luyten half-second proper-motion stars
has resulted in the discovery of an unusual new magnetic white dwarf. LHS 2
534 proves to be the first magnetic DZ, showing Zeeman-split Na I and Mg I
components, as well as Ca I and Ca ii lines for which Zeeman components are
blended. The Na I splittings result in a mean surface field strength estim
ate of 1.92 MG. Apart from the magnetic field, LHS 2534 is one of the most
heavily blanketed and coolest DZ white dwarfs at T-eff similar to 6000 K.