The spectrum of Nova Vulpeculae 1984 No. 2 at nebular phase

Details The spectrum of Nova Vulpeculae 1984 No. 2 at nebular phase The spectrum of Nova Vulpeculae 1984 No. 2 at nebular phase

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..475a&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Astronomy and Astrophysics

Astrophysics

Infrared Spectra, Novae, Stellar Mass Ejection, Stellar Spectrophotometry, Emission Spectra, Forbidden Bands, Near Infrared Radiation, Nebulae, Spectral Line Width, Stellar Temperature

Scientific paper

Nova Vul 1984 No. 2 has been again observed at Observatoire de Haute-Provence in the autumn of 1985, i.e. 270 - 295 days after maximum. It was then in the nebular phase. The spectra cover the blue-violet and the near infrared regions. Over 50 lines and blends have been identified and are given. No clear pattern is observed in the emission bands of a width of about 1450 km/sec. The most conspicuous features observed are the forbidden Ne III and Ne V lines. The infrared region is dominated by a very strong He I 1083 nm emission.

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