The Photometry of V1974 Cyg = N Cyg 1992

Details The Photometry of V1974 Cyg = N Cyg 1992 The Photometry of V1974 Cyg = N Cyg 1992

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..323s&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3

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3

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Photometric, Polarimetric, And Spectroscopic Instrumentation, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays

Scientific paper

The results of photoelectric and CCD U BV RI observations and extensive CCD and TV monitoring of V1974 Cas during the decline phase are shown. Strong features in the ultraviolet light and colour curves are caused by the temporal appearance of forbidden neon emissions. The improved orbital period of 0.08125970(+/-5) day is determined. The ``superhump'' period of 0.08522 day is still observed, too.

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