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   PR # 43025
   We propose ASCA observations of the hybrid BL Lac-OVV quasar object
   B2 1308+326 (z=0.996) in order to determine, on the basis of its
   x-ray spectrum, the true character of this source. It displays strong
   variability, high polarisation and weak line emission, all of which
   led to its classification as a BL Lac object. However, its VLBI
   polarisation structure perpendicular to the jet and association with
   a Fanaroff-Riley II radio galaxy make this classification dubious.
   The known x-ray spectral differences between BL Lacs and both highly
   polarised quasars and flat radio spectrum QSOs provide a means
   whereby the true nature of B2 1308+326 may be deduced. Simultaneous
   optical and radio monitoring will be used to investigate the
   suggestion that this source is a microlensed quasar.
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