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   PR # 41100
   We propose to observe two metal-poor giant elliptical galaxies
   NGC5018 and NGC2865. These galaxies are well known to have unusually
   low Mg2 indices indicating very low metallicity in spite of their
   high luminosity. We wish to confirm first if hot X-ray gas in these
   galaxies show really low iron abundances which suggest they were
   formed by rare mergers bewteen two gas-less ellipticals. Second, and
   if so it means that the observed iron abudance in the gas is
   essentially the same as the mean stellar iron abundance and suggests
   no SNIa contribution to the nucleosynthesis in elliptical galaxies,
   in contrast to the case in the solar neighbourhood of the Milky Way.
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