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We present $Chandra$ ACIS imaging spectroscopy of the nucleus of the Seyfert2 Galaxy Mrk 34. We identify spatially and spectrally resolved features in theband that includes Fe K$\alpha$, Fe XXV and Fe XXVI. These features indicatehigh-velocity ($\gtrsim15,000\,\rm{km\,s}^{-1}$ line-of-sight) materialseparated spanning $\sim$0.5 arcsec, within $\sim200$ pc of the nucleus. Thisoutflow could have deprojected velocities $\sim12-28\times$ greater than the [OIII] emitting outflows, and could potentially dominate the kinetic power in theoutflow. This emission may point to the origins of the optical and X-ray windsobserved at larger radii, and could indicate a link between ultra-fast outflowsand AGN feedback on $\gtrsim$kpc scales.

A UFO Seen Edge-On: Resolving Ultrafast Outflow Emission on $\sim$200-pc Scales with $Chandra$ in the Active Nucleus of Mrk 34