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   PR # 12055
    We propose to make a 40ksec exposure of the G1.5 V star pi1 UMa and a
    20ksec exposure of the G9.5III star beta Cet in order to obtain high-
    quality ASCA spectra (4500 and 12000 cts in each SIS, respectively)
    of these stars,which have been selected because they are single stars
    and bright Xray sources.We note that few high-quality,high-resolution
    X-ray spectra of `normal' solar type stars, either dwarfs or giants,
    have previously been obtained, and argue that such data are needed to
    help in interpreting the X-ray spectra of the active binary stars on
    which previous X-ray spectroscopy have concentrated,by serving as
    reference spectra. We will analyse these two spectra in detail,
    searching for evidence for non-solar abundances and temperature
   stratification.
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