We present pulse profiles of 17 pulsars showing the polarization characteristics at frequencies near 600 MHz. Sixteen of these pulsars were discovered in the second Molonglo survey, while PSR 0529 – 66 is a pulsar in the Large Magellanic Cloud(LMC). The polarization data were analyzed to determine the rotation measures of the pulsars.
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Costa et al. (1991) studied this question.