CCD time-resolved photometry of faint cataclysmic variables. IV

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

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..300h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, March 1991, p. 300-309. Research supported by Lowe

Astronomy and Astrophysics

Astronomy

35

Astronomical Photometry, Cataclysmic Variables, Charge Coupled Devices, Faint Objects, Light Curve, Temporal Resolution, Periodic Variations, Sky Surveys (Astronomy), Stellar Color, White Dwarf Stars

Scientific paper

Time-resolved CCD photometry in V, B, and the near-IR has been obtained, with average time-series length of 3 hours, for 15 certified or candidate cataclysmic-variable faint stars. Orbital periods are found in three of the stars, and nine others are noted to exhibit evidence leading toward confirmation of cataclysmic-variable status. The characteristics of PG 0917+342 and PG 2240+193 are as yet unclear.

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