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Rapid oscillations in cataclysmic variables. 11: X-ray pulses in YY DraconisROSAT observations of the cataclysmic variable YY Draconis reveal pulses with a period of 264.6 + or - 1.2 s, confirming the presence of a rapidly rotating, magnetic white dwarf. Comparison with the periods seen in ultraviolet and blue light indicates that the 275-s ultraviolet signals arises from the reprocessing of X-ray pulsations in structures fixed in the binary reference frame. Only harmonics and orbital sidebands of the white dwarf spin frequency are observed, not the spin frequency itself.
Document ID
19950043644
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Patterson, Joseph
(Columbia Univ. New York, NY, United States)
Szkody, Paula
(Univ. of Washington, Seattle, WA United States)
Date Acquired
August 16, 2013
Publication Date
October 1, 1993
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 105
Issue: 692
ISSN: 0004-6280
Subject Category
Astronomy
Report/Patent Number
ISSN: 0004-6280
Accession Number
95A75243
Funding Number(s)
CONTRACT_GRANT: NAG5-1598
CONTRACT_GRANT: NAG5-1927
Distribution Limits
Public
Copyright
Other

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