CCD time-resolved photometry of faint cataclysmic variables. III

Details CCD time-resolved photometry of faint cataclysmic variables. III CCD time-resolved photometry of faint cataclysmic variables. III

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..758h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, July 1990, p. 758-772. Research supported by NASA.

Astronomy and Astrophysics

Astronomy

41

Cataclysmic Variables, Charge Coupled Devices, Near Infrared Radiation, Stellar Spectrophotometry, Eclipses, Infrared Radiation, Light Curve, Light Modulation

Scientific paper

CCD 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.

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