New Magellan spectra of six low-mass AGN host galaxies yield black hole masses consistent with known scaling relations, and reveal a galaxy with triple-peaked emission lines likely produced by a central AGN outflow plus an extended ring or disk of shocked gas.
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Magellan Spectroscopy of AGNs in Low-mass Galaxies: Scaling Relations and a Triple-Peaked AGN
New Magellan spectra of six low-mass AGN host galaxies yield black hole masses consistent with known scaling relations, and reveal a galaxy with triple-peaked emission lines likely produced by a central AGN outflow plus an extended ring or disk of shocked gas.