Nova Cygni 1992 - Spectral development in the near-infrared at maximum light

Details Nova Cygni 1992 - Spectral development in the near-infrared at maximum light Nova Cygni 1992 - Spectral development in the near-infrared at maximum light

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261l...1a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 1, p. L1-L4.

Astronomy and Astrophysics

Astronomy

7

H Lines, Infrared Spectra, Nitrogen Atoms, Novae, Optical Emission Spectroscopy, Oxygen Spectra, Stellar Spectra, Absorption Spectra, Abundance, Cataclysmic Variables, Emission Spectra, Near Infrared Radiation

Scientific paper

Spectroscopic observations of Nova Cygni 1992 in the range of 0.64-1.15
micron performed from February 22 to 24 are described. A strong increase
of emission in the HI, OI, and NI lines and the onset of the two
absorption systems on February 23 were observed. Indications of a strong
overabundance of nitrogen were found.

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