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   PR # 42100
   We propose to observe the local group galaxy M32 for 30 ksec with
   ASCA. The proximity of M32 provides a unique opportunity to study the
   x-ray properties of a compact elliptical galaxy and extend the
   investigation of the x-ray emission from early-type systems to an
   unprecedented low x-ray-to-optical flux ratio. Because M32 is
   unlikely to retain a hot gas halo, an unimpeded view of the emission
   from the sum of x-ray binaries and/or an AGN associated with the
   central black hole is expected. Previous observations are not
   sufficient to constrain the x-ray spectral parameters.
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