We report on seven peculiar faint blue stars found in the course of th
e Hamburg/ESO survey (HES) which appear to be magnetic white dwarfs (W
Ds) with non-hydrogen spectra. We show in particular that four of them
(HE 0338-3853, HE 0107-0158, HE 0026-2150, and HE 0003-5701) have He
I lines split by magnetic fields of roughly 20 MG, since the pi compon
ents of He I 5876 Angstrom and He I 4929 Angstrom can be identified un
ambiguously in their spectra, and the sigma(+), sigma(-) components ca
n be identified in the spectra of two of these stars (HE 0338-3853 and
HE 0003-5701). Besides GD 229, these are the first magnetic DB white
dwarfs discovered so far. In addition, three further WDs with broad, u
nidentifiable features have been found: HE 1043-0502, HE 0236-2656, an
d HE 0330-0002. We argue that in all three of these stars HI can not b
e responsible for the broad features, and He I most probably not for t
he features in HE0236-2656 and HE 0330-0002, while it still remains po
ssible that the broad features of HE 1043-0502 are due to He I.