  We present and discuss three extremely r-process enhanced stars located in
the massive dwarf spheriodal galaxy Fornax. These stars are very unique with an
extreme Eu enrichment ($1.25\le \mathrm{[Eu/Fe]} \le 1.45$) at high
metallicities ($-1.3 \le \mathrm{[Fe/H]} \le -0.8$). They have the largest Eu
abundances ever observed in a dwarf galaxy opening new opportunities to further
understand the origin of heavy elements formed by the r-process. We derive
stellar abundances of Co, Zr, La, Ce, Pr, Nd, Er, and Lu using 1-dimensional,
local thermodynamic equilibrium (LTE) codes and model atmospheres in
conjunction with state-of-the art yield predictions. We derive Zr in the
largest sample of stars (105) known to date in a dwarf galaxy. Accurate stellar
abundances combined with a careful assessment of the yield predictions have
revealed three metal-rich stars in Fornax showing a pure r-process pattern. We
define a new class of stars, namely Eu-stars, as r-II stars (i.e., [Eu/Fe]$>1$)
at high metallicities (i.e., $\mathrm{[Fe/H]}\gtrsim -1.5$). The stellar
abundance pattern contains Lu, observed for the first time in a dwarf galaxy,
and reveals that a late burst of star formation has facilitated extreme
r-process enhancement late in the galaxy's history ($<4$\,Gyr ago). Due to the
large uncertainties associated with the nuclear physics input in the yield
predictions, we cannot yet determine the r-process site leading to the three
Eu-stars in Fornax. Our results demonstrate that extremely r-rich stars are not
only associated with ultra faint low-mass dwarf galaxies, but can be born also
in massive dwarf galaxies.
