Far-ultraviolet spectroscopy of O+O binaries in the Magellanic Clouds

We report FUSE observations in 2005–2006 of three O-type, double-lined spectroscopic binaries in the Magellanic Clouds. The systems have very short periods (1.4–2.25 d), represent rare, young evolutionary stages of massive stars and binaries, and provide a unique glimpse at some of the most massive...

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Bibliographic Details
Main Authors: Iping, R.C., Sonneborn, G., Massa, D.L., Gies, D., Williams, S.
Format: Others
Language:English
Published: Universität Potsdam 2007
Subjects:
Online Access:http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17896
http://opus.kobv.de/ubp/volltexte/2008/1789/