The system SBS 0909+532A, B is a double consisting of a quasar and a f
ainter component that was, until now, spectroscopically unresolved. Sp
ectra taken in good seeing conditions (FWHM = 1 '') with the 4.2 m Wil
liam Herschel Telescope separate the A and B components, showing that
both are quasars with the same redshift, z = 1.377, and identical spec
tra. Consequently, this supports the gravitational lens interpretation
of SBS 0909+532. The ME II lambda lambda 2796, 2803 doublet is found
in absorption at the same redshift (z = 0.83) in both components, alth
ough the equivalent width of the faintest one is 3 times stronger. We
discuss the possibility that these absorption features arise from the
photometrically unidentified lensing galaxy. We have also observed ano
ther double system, Q1222+226, which was recently reported to be a gra
vitationally lensed quasar. Comparison of the spectra of both componen
ts indicates that Q1222+226 is in fact composed of a quasar and a star
.