  We present the results of a search for metal absorption lines in the spectra
of background QSOs whose sightlines pass close to foreground QSOs. We detect
MgII(2796,2803) absorption in Sloan Digital Sky Survey (SDSS) spectra of four
z>1.5 QSOs whose lines of sight pass within 26-98 kpc of lower redshift
(z~0.5-1.5) QSOs. The 100% [4/4 pairs] detection of MgII in the background QSOs
is clearly at odds with the incidence of associated (z_abs ~ z_em) systems --
absorbers which exist towards only a few percent of QSOs. Although the quality
of our foreground QSO spectra is not as high as the SDSS data, absorption seen
towards one of the background QSOs clearly does not show up at the same
strength in the spectrum of the corresponding foreground QSO. This implies that
the absorbing gas is distributed inhomogeneously around the QSO, presumably as
a direct consequence of the anisotropic emission from the central AGN. We
discuss possible origins for the MgII lines, including: absorption by gas from
the foreground QSO host galaxy; companion galaxies fuelling the QSO through
gravitational interactions; and tidal debris left by galaxy mergers or
interactions which initiated the QSO activity. No single explanation is
entirely satisfactory, and we may well be seeing a mixture of phenomena.
