New spectroscopy of NGC 2366 shows Mrk 71 and its outflow are more oxygen-rich than other HII regions, and identifies new Wolf-Rayet and supernova remnant candidates.
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Chemical abundances and small-scale gas kinematics in the local star-forming galaxy NGC 2366
New spectroscopy of NGC 2366 shows Mrk 71 and its outflow are more oxygen-rich than other HII regions, and identifies new Wolf-Rayet and supernova remnant candidates.