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Polarimetry of magnetic cataclysmic variables

Bibliography: pages 136-138.

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Main Author: Cropper, Mark Scott
Other Authors: Warner, Brian
Format: Thesis
Language:English
Published: Department of Astronomy 2016
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access_status_str Open Access
author Cropper, Mark Scott
author2 Warner, Brian
author_browse Cropper, Mark Scott
Warner, Brian
author_facet Warner, Brian
Cropper, Mark Scott
author_sort Cropper, Mark Scott
collection Thesis
description Bibliography: pages 136-138.
format Thesis
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institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:49:30.041Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2016
publishDateRange 2016
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publisher Department of Astronomy
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source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/17034 Polarimetry of magnetic cataclysmic variables Cropper, Mark Scott Warner, Brian Astronomy Bibliography: pages 136-138. The design and construction of an astronomical polarimeter is described and an evaluation made of its performance. Extensive observations of cataclysmic variables with emphasis on the AM Her and DQ Her classes are then presented. After consideration of the basic principles involved in the development of an efficient and accurate polarimeter, a design using two super-achromatic retarders (a 1/4 wave and a 1/2 wave) rotating above a fixed analyser was adopted. This permitted simultaneous linear and circular polarisation measurements, or, by rearranging the order of the retarders in the beam, linear polarisation measurements alone, or circular polarisation measurements alone, with enhanced efficiency. The polarimeter was found to have extremely low instrumental polarisations and, because of the superachromatic retarders used, the efficiency correction factors were very close to 1 at all wavelengths. The polarisations are calculated at the telescope and the light curve at a higher time resolution may also be recorded if this is required. Extensive sets of observations using the polarimeter were obtained for six of the ten AM Her variables (or "polars"). EF Eri and El405-451 were observed most. Evidence was found in El405-451 for movement of the apparent location of the accretion region on the primary star and the inclination and magnetic dipole off set from the rotation axis was determined. This allowed a comparison to be made between the competing models for the cyclotron emission, showing that those which take into account the temperature structure of the accretion region provide the best results. Observations and an analysis of the polarisation data from H0139-68, E2003+225, VV Puppis and PG1550+191 are also presented in some detail. A final chapter presents results from observations made to detect a modulation in the polarisation at the rotation period of the primary in the DQ Her variables. Upper limits are set for 4 members of the class and the implications of the results are discussed. 2016-02-15T07:15:09Z 2016-02-15T07:15:09Z 1985 Doctoral Thesis Doctoral PhD http://hdl.handle.net/11427/17034 eng application/pdf Department of Astronomy Faculty of Science University of Cape Town
spellingShingle Astronomy
Cropper, Mark Scott
Polarimetry of magnetic cataclysmic variables
thesis_degree_str Doctoral
title Polarimetry of magnetic cataclysmic variables
title_full Polarimetry of magnetic cataclysmic variables
title_fullStr Polarimetry of magnetic cataclysmic variables
title_full_unstemmed Polarimetry of magnetic cataclysmic variables
title_short Polarimetry of magnetic cataclysmic variables
title_sort polarimetry of magnetic cataclysmic variables
topic Astronomy
url http://hdl.handle.net/11427/17034
work_keys_str_mv AT croppermarkscott polarimetryofmagneticcataclysmicvariables