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Redshifted Cool Gas in the Disturbed HI Disk of the Starburst Dwarf NGC 4214
We report redshifted cool gas toward the central star-forming region of the nearby starburst dwarf galaxy NGC 4214. HST/COS spectra show low-ionization absorbers redshifted relative to the systemic velocity, most clearly in SII ($Δv=19.8\pm2.6\ {\rm km\,s^{-1}}$) and supported by MgII ($Δv=30.3\pm3.
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