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A Search for Hot Subdwarf Companions to Rapidly-Rotating Early B Stars
Published online by Cambridge University Press: 23 January 2015
Abstract
We continue to search for O-type subdwarf companions in binary systems containing Be primaries. We were not able to confirm an sdO object in π Aqr and HR 2142, even though optical and UV observations suggest their presence. Some possible reasons are enumerated.
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- Copyright © International Astronomical Union 2015