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   62126
   We propose a 40 ks Asca observation of Seyfert 2 galaxy NGC 513 in
   order to measure its nuclear emission as well as the scattered
   component. This source is the only one of 10 Seyfert 2s with broad line
   flux measured in the polarized light - and thus harboring an AGN - but
   with no sensitive soft or hard X-ray observations. The measurement - or
   even a limit - on its X-ray flux will allow us to compare the
   properties of the scatterer as measured in the polarized light to that
   measured in soft X-rays, which is crucial for diagnostics of the
   putative scettering medium present in the "Unified schemes" for the two
   types of Seyferts.
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