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HE 0141-3932 (zem = 1.80) is a bright blue radio-quite quasar with anunusually weak Ly-alpha emission line. Large redshift differences (Delta z =0.05) are observed between high ionization and low ionization emission lines.Absorption systems identified at zabs = 1.78, 1.71, and 1.68 show mildoversolar metallicities (Z ~= 1-2Zsolar) and can be attributed to theassociated gas clouds ejected from the circumnuclear region. The joint analysisof the emission and absorption lines leads to the conclusion that this quasaris seen almost pole-on. Its apparent luminosity may be Doppler boosted by ~10times. The absorbing gas shows a high abundance of Fe, Mg and Al ([Fe, Mg,Al/C] ~= 0.15 +/- 0.10) along with underabundance of N ([N/C] <= -0.5). Thisabundance pattern is at variance with current chemical evolution models of QSOspredicting [N/C] >= 0$ and [Fe/C] < 0 at Z ~ Zsolar.Comment: 12 pages, 6 figures, accepted for publication in A&

HE 0141-3932: A bright QSO with an unusual emission line spectrum and associated absorption