The R-Process Alliance: J1521-3538, a very metal-poor, extremely
  r-process-enhanced star with [Eu/Fe]=+2.2, and the class of r-III stars
  We report the discovery of J1521-3538, a bright (V=12.2), very metal-poor
([Fe/H]=-2.8) strongly r-process enhanced field horizontal branch star, based
on a high-resolution, high signal-to-noise Magellan/MIKE spectrum. J1521-3538
shows the largest r-process element over-abundance in any known
r-process-enhanced star, with [Eu/Fe]=+2.2, and its chemical abundances of 22
neutron-capture elements closely match the scaled solar r-process pattern.
J1521-3538 is also one of few known carbon-enhanced metal-poor stars with
r-process enhancement (CEMP-r stars), as found after correcting the measured C
abundance for the star's evolutionary status. We propose to extend the existing
classification of moderately enhanced (+0.3<=[Eu/Fe]<=+1.0) r-I and strongly
r-process enhanced ([Eu/Fe]>+1.0) r-II stars to include an r-III class, for
r-process stars such as J1521-3538, with [Eu/Fe]>+2.0 and [Ba/Eu]<-0.5, or >100
times the solar ratio of europium to iron. Using cosmochronometry, we estimate
J1521-3538 to be 12.5+-5 Gyr and 8.9+-5 Gyr old, using two different sets of
initial production ratios. These ages are based on measurements of the Th line
at 4019 A and other r-process element abundances. This is broadly consistent
with the old age of a low-mass metal-poor field red horizontal branch star.
J1521-3538 likely originated in a low-mass dwarf galaxy that was later accreted
by the Milky Way, as evidenced by its highly eccentric orbit.
