Physics
Scientific paper
Sep 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msngr.129...53c&link_type=abstract
The Messenger, vol. 129, p. 53-57
Physics
1
Scientific paper
Wolf-Rayet (WR) stars are the chemical-ly evolved descendents of O stars, such that they trace massive star formation. Here we present results of recent VLT/FORS surveys of WR stars in near- by spiral and irregular galaxies and consider individual WR stars as progenitors of Type Ib/c core-collapse supernovae. Young massive clusters hosting large WR populations may be used as templates for high-redshift Lyman break galaxies.
Crowther Paul A.
Hadfield Lucy J.
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