A CH star in the globular cluster NGC 6426
  We report on the serendipitous discovery of a carbon star near the centre of
the low-metallicity globular cluster NGC 6426. We determined its membership and
chemical properties using medium-resolution spectra. The radial velocity of
-159 km/s makes it a member of the cluster. We used photometric data from the
literature and the COMARCS stellar atmospheric models to derive its luminosity,
effective temperature, surface gravity, metallicity, and approximate C, N, and
O abundance ratios. According to these properties, we suggest that this star is
a genuine carbon rich low-metallicity AGB star.
