HD 202383

UBV observations of V1500 Cyg. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1977PASP...89...44W&db_key=AST
Photometric observations of Nova V1500 Cygni UBV photometric observations of Nova Cygni 1975 = V1500 Cygni wereobtained in the time interval from September 1975 to October 1976. Theshort-period variability discovered by Tempesti (1975) and Koch andAmbruster (1975) has always been present but with greatly varyingamplitude in a range from 0.03 to 0.7 mag. The period decreased from0.1410 day in September 1975, when the short-term variations were firstdiscovered, to 0.1380 day in autumn 1976. The roughly sinusoidal lightcurve changes its shape from cycle to cycle, and there are irregularfluctuations superposed.
Light curve of Nova V1500 CYG 1975. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1976ApJ...209..882Y&db_key=AST
A Short Period Light Variation in Nova Cygni 1975 Not Available

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