Nova Cygni 1978. I - The nebular phase

Details Nova Cygni 1978. I - The nebular phase Nova Cygni 1978. I - The nebular phase

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..107s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 197, Oct. 1981, p. 107-138.

Astronomy and Astrophysics

Astronomy

98

Cygnus Constellation, Emission Spectra, Line Spectra, Nebulae, Ultraviolet Astronomy, Abundance, Infrared Astronomy, Interstellar Extinction, Iue, Luminous Intensity, Nuclear Fusion, Resonance Lines, Stellar Mass Ejection

Scientific paper

UV observations of Nova Cygni 1978 have been obtained using IUE on 17 dates between 1978 September 12 and 1979 July 8 inclusive. The discussion includes the interpretation, during the nebular stage, of the UV observations together with optical and IR data from other observers. Analysis of the available data indicates that Nova Cygni 1978 was produced by a mechanism involving a thermonuclear runaway.

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