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Guest observer program OAOThe OAO-A2 observations of two Be stars, 60 Cygnus and gamma Cassiopeia, were analyzed. It is shown that unpolarized radiation produced by continuous Balmer emission in the atmospheres of Be stars is significant in the explanation of the polarization observed below the Balmer discontinuity. Available multicolor polarimetry data was also analyzed with respect to interstellar polarization.
Document ID
19730003101
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Coyne, G. V. (Arizona Univ. Tucson, AZ, United States)
Date Acquired
September 2, 2013
Publication Date
August 29, 1972
Subject Category
Space Sciences
Report/Patent Number
NASA-CR-129166
Report Number: NASA-CR-129166
Accession Number
73N11828
Funding Number(s)
CONTRACT_GRANT: NGR-03-002-193
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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