Chemical abundances in bright giants of the globular cluster M62 (NGC
  6266)
  With the exception of Terzan 5, all the Galactic globular clusters that
possess significant metallicity spreads, such as omega Cen and M22, are
preferentially the more luminous clusters with extended horizontal branches.
Here we present radial velocities and chemical abundances for seven bright
giants in the globular cluster M62, a previously little-studied cluster. With
M_V = -9.18, M62 is the ninth most luminous Galactic globular cluster and has
an extended horizontal branch. Within our sample, we find (i) no evidence for a
dispersion in metallicity, [Fe/H], beyond the measurement uncertainties, (ii)
star-to-star abundance variations for C, O, Na and Al with the usual
correlations between these elements as seen in other globular clusters, and
(iii) a global enrichment for the elements Zr, Ba and La at the level [X/Fe] =
+0.4 dex. For elements heavier than La, the abundance ratios are consistent
with the scaled-solar $r$-process distribution. Below La, the abundances are
anomalous when compared to the scaled-solar s-process or r-process
distributions. For these elements, the abundance signature in M62 is in
agreement with predictions of the s-process from fast-rotating massive stars,
although the high [Rb/Y] ratio we measure may be a challenge to this scenario.
