A far red spectrum of Nova LMC 1981

Details A far red spectrum of Nova LMC 1981 A far red spectrum of Nova LMC 1981

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...124..143a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 124, no. 1, July 1983, p. 143-146.

Astronomy and Astrophysics

Astrophysics

1

Infrared Spectra, Magellanic Clouds, Novae, Stellar Spectra, Visible Spectrum, Helium, Hydrogen, Line Spectra, Oxygen, Paschen Series, Spectrum Analysis

Scientific paper

A far red spectrum (6000-10,000 Å) of Nova LMC 1981 has been obtained at a phase roughly 70 d after presumed maximum. The prominent lines seen are the Paschen series of hydrogen, He I 7065 Å and O I 8446 Å. Comparison with similar spectra of several Galactic Novae shows that we are dealing with a fast nova probably just entering the nebular phase. A striking resemblance exists with Nova Cyg 1975, 72 d after maximum, with the notable exception of the [O II] lines absent in Nova LMC.

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