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Predictions for arc polarizationMaps for the prediction of the polarization of light echo arcs are presented. It is noted that the results can be compared with observations in order to test the light-echo model of Katz (1987) and Milgrom (1987) and to determine its parameters. As long as the model assumptions of single scattering and planar geometry remain valid, the polarization is shown to be independent of the geometrical thickness and the optical depth of the dust layer. Cases such as the light source being in the plane of scatterers and arcs consisting of nearly forward scattered light are considered.
Document ID
19880058322
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Katz, J. I.
(Washington Univ. Saint Louis, MO, United States)
Jackson, S.
(Washington University Saint Louis, MO, United States)
Date Acquired
August 13, 2013
Publication Date
May 1, 1988
Publication Information
Publication: Astronomy and Astrophysics
Volume: 197
Issue: 1-2
ISSN: 0004-6361
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-6361
Accession Number
88A45549
Funding Number(s)
CONTRACT_GRANT: NSF AST-84-12895
Distribution Limits
Public
Copyright
Other

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