Photometric variability of 1329-294

Details Photometric variability of 1329-294 Photometric variability of 1329-294

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..667k&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, July 1989, p. 667, 668.

Physics

4

Blue Stars, Cataclysmic Variables, Dwarf Novae, Stellar Physics, Stellar Spectrophotometry, Charge Coupled Devices, Light Curve, Visual Photometry

Scientific paper

The V-band CCD photometry of a faint cataclysmic variable 1329-294
revealed its periodic light variations with the most likely period of
3.8 hours. No eclipse was seen. Known characteristics of this system
suggest that it is a dwarf nova.

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