Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..169h&link_type=abstract
Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2
Astronomy and Astrophysics
Astronomy
Scientific paper
New NTT/SOFI near-IR narrow-band imaging and spectroscopy reveals an additional four Wolf-Rayet (WR) stars in the massive cluster Westerlund 1, bringing the total WR population to 24. Sixteen of the WR stars in Wd1 have been classified WN5--11, while eight are WC8--9. An observed WR to RSG/YHG ratio of ˜3 suggests an age of 4.5--5.0 Myr, with WR stars descended from 40--55Msun progenitors. On the basis of dust and hard X-ray emission, we estimate that 40--65% are probable members of massive star binary systems.
Clark Simon J.
Crowther Paul A.
Hadfield Lucy J.
Negueruela Ignacio
Vacca William D.
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