The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster
本文档由 飞亚 分享于2010-12-29 15:35
We combine new CCD UBV photometry and spectroscopy with that from the nliterature to investigate 19 Magellanic Cloud OB associations that contain nWolf-Rayet (WR) and other types of evolved massive stars. Our spectroscopy nreveals a wealth of newly identified interesting objects, including early nO-type supergiants, a high mass double-lined binary in the S..
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