The Morphology of a Mass Loss Episode of the Be Star w Orionis.

Intensive optical photometry and linear polarimetry have detailed the morphology of a recent mass-loss episode of the Be star Omega Orionis. The continuum photometry and polarimetry were found to change in close concert. The H-alpha line photometry and polarimetry were also correlated, albeit to a l...

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Bibliographic Details
Main Authors: Hayes, Daniel P., Guinan, Edward F.
Format: Villanova Faculty Authorship
Published: 1983
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