arXiv · 2209.14326
A UFO Seen Edge-On: Resolving Ultrafast Outflow Emission on $\sim$200-pc Scales with $Chandra$ in the Active Nucleus of Mrk 34
Abstract
We present $Chandra$ ACIS imaging spectroscopy of the nucleus of the Seyfert 2 Galaxy Mrk 34. We identify spatially and spectrally resolved features in the band that includes Fe K$\alpha$, Fe XXV and Fe XXVI. These features indicate high-velocity ($\gtrsim15,000\,\rm{km\,s}^{-1}$ line-of-sight) material separated spanning $\sim$0.5 arcsec, within $\sim200$ pc of the nucleus. This outflow could have deprojected velocities $\sim12-28\times$ greater than the [O III] emitting outflows, and could potentially dominate the kinetic power in the outflow. This emission may point to the origins of the optical and X-ray winds observed at larger radii, and could indicate a link between ultra-fast outflows and AGN feedback on $\gtrsim$kpc scales.
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W. Peter Maksym, Martin Elvis, Giuseppina Fabbiano, Anna Trindade-Falcão, Steven B. Kraemer, Travis C. Fischer, D. Michael Crenshaw, Thaisa Storchi-Bergmann. 2022-09-28. A UFO Seen Edge-On: Resolving Ultrafast Outflow Emission on $\sim$200-pc Scales with $Chandra$ in the Active Nucleus of Mrk 34. https://arxiv.org/abs/2209.14326
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