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   62074
   G~70.7+1.2 is a region of radio nebulosity containing a bright infra-
   red star with a unique emission spectrum. Its non-thermal radio
   spectrum is indicative of a central source of relativistic particles,
   eg., a pulsar. The observations are best interpreted in terms of a
   binary with a neutron star component plowing through dense interstellar
   medium. We propose to observe G~70.7+1.2 for 40-ks with ASCA. X-ray
   spectroscopy is the best way to elucidate the enigma of G~70.7+1.2 in
   terms of either and accreting neutron star or a rotation powered
   pulsar.
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