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...
| Main Authors: | , |
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| Format: | |
| Language: | English |
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1983
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| Online Access: | http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176586 |