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   63005
   We propose to observe two well known, X-ray bright dMe flare stars,
   Wolf 630 and EV Lac. Neither of them has been observed so far with
   ASCA, yet they are ideal targets, thanks also to the coming
   availability of their SAX observations, for the study of the
   temperature structures, as well as for the coronal abundance patterns,
   in this class of stars in which coronal activity reaches its most
   extreme levels compared to their modest optical luminosity. The
   proposed observations will allow sufficient statistics to be
   accumulated to allow a detailed analysis in terms of loop models, as
   well as to put solid constraints (together with the recent reliable
   photospheric analyses of M dwarfs photospheric abundance) on the
   presence of eventual coronal abundance anomalies.
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