UBV photometry of close visual double stars using an area scanner

A computer-controlled area scanner designed for use on close visual double stars is described. Techniques used in making observations and in subsequent reduction of the data are given. Problems encountered are discussed. Magnitude differences and magnitudes and colours of components are given for 15...

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Bibliographic Details
Main Author: Hurly, Patrick Rupert
Other Authors: Warner, Brian
Format: Dissertation
Language:English
Published: University of Cape Town 2016
Subjects:
Online Access:http://hdl.handle.net/11427/16638
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spelling ndltd-netd.ac.za-oai-union.ndltd.org-uct-oai-localhost-11427-166382020-10-06T05:10:58Z UBV photometry of close visual double stars using an area scanner Hurly, Patrick Rupert Warner, Brian Astronomy A computer-controlled area scanner designed for use on close visual double stars is described. Techniques used in making observations and in subsequent reduction of the data are given. Problems encountered are discussed. Magnitude differences and magnitudes and colours of components are given for 153 bright southern close visual doubles. Separations are given for some of the stars. Absolute magnitudes are calculated for the primaries by several methods. Individual stars are discussed where appropriate. The accuracy of the results is discussed. No significant systematic errors are evident in the results, but systematic errors are present in the results of other authors. Suggestions are made for the future use of conventional photometers, scanners and other techniques in the field of visual double star photometry and astrometry. 2016-02-01T10:02:48Z 2016-02-01T10:02:48Z 1976 Master Thesis Masters MSc http://hdl.handle.net/11427/16638 eng application/pdf University of Cape Town Faculty of Science Department of Astronomy
collection NDLTD
language English
format Dissertation
sources NDLTD
topic Astronomy
spellingShingle Astronomy
Hurly, Patrick Rupert
UBV photometry of close visual double stars using an area scanner
description A computer-controlled area scanner designed for use on close visual double stars is described. Techniques used in making observations and in subsequent reduction of the data are given. Problems encountered are discussed. Magnitude differences and magnitudes and colours of components are given for 153 bright southern close visual doubles. Separations are given for some of the stars. Absolute magnitudes are calculated for the primaries by several methods. Individual stars are discussed where appropriate. The accuracy of the results is discussed. No significant systematic errors are evident in the results, but systematic errors are present in the results of other authors. Suggestions are made for the future use of conventional photometers, scanners and other techniques in the field of visual double star photometry and astrometry.
author2 Warner, Brian
author_facet Warner, Brian
Hurly, Patrick Rupert
author Hurly, Patrick Rupert
author_sort Hurly, Patrick Rupert
title UBV photometry of close visual double stars using an area scanner
title_short UBV photometry of close visual double stars using an area scanner
title_full UBV photometry of close visual double stars using an area scanner
title_fullStr UBV photometry of close visual double stars using an area scanner
title_full_unstemmed UBV photometry of close visual double stars using an area scanner
title_sort ubv photometry of close visual double stars using an area scanner
publisher University of Cape Town
publishDate 2016
url http://hdl.handle.net/11427/16638
work_keys_str_mv AT hurlypatrickrupert ubvphotometryofclosevisualdoublestarsusinganareascanner
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