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Paper: How Extreme are the WR Clusters in NGC 3125?
Volume: 353, Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology
Page: 247
Authors: Hadfield, L.J; Crowther, P.A.
Abstract: We present new VLT/FORS1 imaging and spectroscopy of NGC 3125-A and -B to study their Wolf-Rayet content. From archival HST/STIS and HST/FOC imaging, both regions host two clusters, with the optically fainter cluster of region A heavily reddened. Previously discrepant UV and optical studies of region A are reconciled by a lower reddening. Derived WR populations are in line with expectations for an LMC-metallicity starburst.
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