NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
CCD time-resolved photometry of faint cataclysmic variables. IIICCD time-resolved photometry in V, B, and near-IR for 17 faint cataclysmic variables (CVs) is presented and analyzed. The data are obtained at Kitt Peak National Observatory, the Perkins reflector, Lowell Observatory, and the Observatorio del Roque de los Muchachos from April-June 1989. The degree of variability and periodicities for the CVs are examined. It is observed that the variability of most of the stars is consistent with CV class behavior. Orbital periods for five CVs are determined, and three potential eclipsing systems are detected.
Document ID
19900056602
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Howell, Steve B.
(Planetary Science Institute Tucson, AZ, United States)
Szkody, Paula
(Washington, University Seattle, United States)
Kreidl, Tobias J.
(Lowell Observatory Flagstaff, AZ, United States)
Mason, Keith O.
(Planetary Science Inst. Tucson, AZ, United States)
Puchnarewicz, E. M.
(London, University College, Dorking, United Kingdom)
Date Acquired
August 14, 2013
Publication Date
July 1, 1990
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 102
ISSN: 0004-6280
Subject Category
Astronomy
Accession Number
90A43657
Funding Number(s)
CONTRACT_GRANT: NSF AST-89-15445
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available