galaxy counterpart – if this population has similar star formation properties as AGC 226067, it implies $\sim$0.1 $M_{\odot}$ yr$^{-1}$ in Virgo intracluster star formation. Given its unusual stellar population, AGC 226067 is likely a stripped remnant and is plausibly the result of compressed gas from the ram pressure stripped M86 subgroup ($\sim$350 kpc away in projection) as it falls into the Virgo Cluster.'
author:
- 'D. J. Sand,$\!$ A. C. Seth,$\!$ D. Crnojević,$\!$ K. Spekkens,$\!$ J. Strader,$\!$ E. A. K. Adams,$\!$ N. Caldwell,$\!$ P. Guhathakurta, J. Kenney, S. Randall, J. D. Simon, E. Toloba, B. Willman$\!$'
title: '[*Hubble Space Telescope*]{} Imaging of the Ultra-Compact High Velocity Cloud AGC 226067: A stripped remnant in the Virgo Cluster'
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Introduction
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Searching for faint, isolated dwarf galaxies in large area HI surveys has a long history [see @HIreview for a review]. Most recently, so-called Ultra-Compact High Velocity Clouds (UCHVCs) of neutral hydrogen have been identified by the Galactic Arecibo $L$-Band Feed Array HI (GALFA-HI) and Arecibo Legacy Fast Arecibo $L$-Band Feed Array (ALFALFA) surveys [@Saul12; @Adams13 respectively] as potential sites of gas-bearing dark matter halos. Because the spatial distribution and physical properties of these UCHVCs are consistent with some being faint dwarf 