  Here we present a new bowshock blue-shifted source in the close vicinity of
Sgr A* that we name X8. We use data-sets that are based on SINFONI observations
with the Very Large Telescope. We can trace the source between 2006 and 2016 in
the blue-shifted line maps and it shows not only positional similarities to X7
but also the same spectral footprint. The symmetry axis of both extended
sources points towards Sgr A* and exhibits [Fe III] emission lines that arise
due to wind-wind shocks. In particular, the source X8 has a bipolar morphology,
which makes it the closest bipolar source in the vicinity of Sgr A*. In
addition, we can trace a K-band continuum counterpart of X8. This points
towards a stellar counterpart to the line-map emission. Overall, the source X8
can be interpreted as either a Young Stellar Object or a young planetary
nebula, which makes this source unique among so-far detected main-sequence OB
stars in this region.
