How extreme are the WR clusters in NGC 3125?

Details How extreme are the WR clusters in NGC 3125? How extreme are the WR clusters in NGC 3125?

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..247h&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Physics

Scientific paper

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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