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SS Bootis - A totally eclipsing binary of the RS CVn typePhotoelectric photometry gathered for SS Bootis over the 1976-1981 period shows a distortion wave amplitude variation from 0.05 to 0.20 mag, with no apparent pattern. From the rectified light curve, a new time of midprimary eclipse was found to be 2444332.0335 + or - 0.0005 days. Solutions of the primary eclipse data, rectified for star spots as well as for ellipticity and reflection, are presented.
Document ID
19830060980
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Vaucher, C. A. (Dyer Observatory Nashville, TN, United States)
Africano, J. L. (Cloudcroft Observatory Cloudcroft, NM, United States)
Henry, G. W. (Dyer Observatory Nashville, TN, United States)
Hall, D. S. (Dyer Observatory Nashville, TN, United States)
Wilson, J. W. (Dyer Observatory Nashville, TN, United States)
Date Acquired
August 11, 2013
Publication Date
August 1, 1983
Publication Information
Publication: Astronomical Journal
Volume: 88
ISSN: 0004-6256
Subject Category
Astrophysics
Accession Number
83A42198
Funding Number(s)
PROJECT: AF PROJECT ESD-0-0935
OTHER: NSG-7543
Distribution Limits
Public
Copyright
Other

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