The spectrum of U Scorpii in the 1987 outburst

Details The spectrum of U Scorpii in the 1987 outburst The spectrum of U Scorpii in the 1987 outburst

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...201...89r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 201, no. 1, July 1988, p. 89-92.

Astronomy and Astrophysics

Astrophysics

12

Emission Spectra, Novae, Scorpius Constellation, Stellar Spectra, Helium Ions, Hydrogen, Nitrogen Ions, Stellar Composition

Scientific paper

The principal results are given of the spectroscopic observations of the recurrent nova U Sco carried out at Asiago eight and nine days after the maximum of its 1987 outburst. The spectra show emission lines of H, He II, N III and other ions. In spite of the very high degree of excitation, they do not show any traces of forbidden lines. A comparison to the spectra on the outburst in 1979 is given. Some comments follow.

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