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   PR #    95
   The nearby (3.5 Mpc) face-on spiral galaxy NGC1313 contains 3
   intriguing sources, all with soft X-ray luminosities around 10**40
   erg/s, and separated from one another by 6 arcmin. The first is near
   but not coincident with the optical nucleus, and shows a spectrum
   consistent with that of a LINER's. The second has shown flux
   variability of a factor of 2 over 12 years, and is thought to be the
   most luminous known X-ray binary. The third is SN1978K, the first
   supernova to be identified as such on the basis of its X-ray emission.
   An ASCA observation will simultaneously yield the specta of all three
   objects, and allow a determination of their emission mechanism and
   hence their nature.
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