Neon forbidden lines in Nova AQL 1982

Details Neon forbidden lines in Nova AQL 1982 Neon forbidden lines in Nova AQL 1982

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203p...5a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 203, Apr. 1983, p. 5P-8P.

Astronomy and Astrophysics

Astronomy

3

Forbidden Transitions, Neon, Novae, Stellar Spectra, Emission Spectra, Spectral Line Width, Sulfur

Scientific paper

The author presents a spectrum of Nova Aql 1982 obtained 179 days after its discvovery. It shows a very faint continuum with several broad emission lines. In particular [S II] λλ4086-4076, [Ne III] λ3868 and [Ne V] λ3426 are the strongest ones and exhibit a complex structure characterized by eight main components with sometimes secondary components. The full widths are very large, about 6000 km s-1, but they are decreasing with time.

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