The spectrum of Nova Sagittarii 1982 in the transition phase

Details The spectrum of Nova Sagittarii 1982 in the transition phase The spectrum of Nova Sagittarii 1982 in the transition phase

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95..506i&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 95, Aug. 1983, p. 506-508.

Astronomy and Astrophysics

Astronomy

8

Balmer Series, Light Curve, Novae, Stellar Spectra, Variable Stars, Emission Spectra, Stellar Magnitude

Scientific paper

Spectroscopic observations of Nova Sgr 1982 made in October and November, 1982, with a one-prism spectrograph equipped with an S-20 image tube (dispersion 60 A/mm at H-gamma) on 103a-O plates using the 122-cm telescope at Asiago, Italy, are reported. The identifications and relative intensities of the lines from 4100 to 8500 A are presented in a table. Wide Balmer emissions and bright lines of O I, N II, and Fe II are present, indicating that the nova was in a late transitional phase before it disappeared behind the sun. A visual light curve for October and November, 1982, and a sample spectrum are shown.

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