Near-infrared spectrum of Nova Cygni 1975

Details Near-infrared spectrum of Nova Cygni 1975 Near-infrared spectrum of Nova Cygni 1975

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21..327k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 54, May-June 1977, p. 575-579.) Soviet Astronomy, vol. 21, May-June 1977, p. 327-329. Translati

Astronomy and Astrophysics

Astronomy

1

Infrared Astronomy, Near Infrared Radiation, Novae, Stellar Spectra, Cygnus Constellation, Electrophotometry, Emission Spectra, Forbidden Bands, Planetary Nebulae

Scientific paper

Observations of the spectrum of Nova Cyg 1975 in the region from 6000 to 11,000 A are presented, consisting of photoelectric scans made on September 3-4 and 18-19, 1975, and spectrograms taken on September 25-26, 1975. For most of emission lines identified in the spectrum, the absolute flux and equivalent width are determined. The emission-line spectrum of the nova obtained on September 3-4, 1975, was due to H I, He I, N I, O I, C I, and S I. The forbidden lines of N I, O I, O II, and S III marking the nebular stage of the nova appeared in the spectrum of September 18-19, 1975.

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