Nova Cygni 1975

Details Nova Cygni 1975 Nova Cygni 1975

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976poast..24...51w&link_type=abstract

Postepy Astronomii, vol. 24, Jan.-Mar. 1976, p. 51-58. In Polish.

Astronomy and Astrophysics

Astronomy

Cygnus Constellation, Light Curve, Novae, Stellar Evolution, Stellar Spectrophotometry, Emission Spectra, Spectral Line Width, Spectrum Analysis, Universal Time

Scientific paper

The photometric and spectrographic features of the Nova in Cygnus, its discovery in 1975 by Japanese and Polish astronomers, and a Canadian Copernicus Spectrograph employed in observations of the event are described. The first six weeks of the Nova's evolution are reviewed and light-curves are presented. The possibility that the object is a supernova, or a virgin nova (experiencing its first outburst), is considered. Emission lines of four-fold structure and the brightness variations of this unusually fast Nova are examined. The expansion of the Nova shell in the initial evolutionary phase is analyzed.

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