Nova in Cygnus of record brightness

Computer Science

Scientific paper

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Light Curve, Novae, Stellar Spectrophotometry, Ubv Spectra, Milky Way Galaxy, Stellar Luminosity, Stellar Mass Ejection, Supernovae

Scientific paper

Photoelectric UBV observations have been made and a number of intermediate-dispersion spectrograms have been obtained in connection with a study of the recent bright nova in Cygnus. A preliminary light curve is presented. The light curve is smooth during maximum and early decline, but significant fluctuations appear during the transition stage. It is pointed out that a week after maximum most of the light comes from very broad, multiple-component emission lines.

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