The spectrum of Nova Scuti 1975

Details The spectrum of Nova Scuti 1975 The spectrum of Nova Scuti 1975

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975crasb.281..169f&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie B - Sciences Physiques, vol. 281, no. 11, Sept. 15, 1975, p. 169-172. In F

Astronomy and Astrophysics

Astronomy

3

Emission Spectra, Infrared Astronomy, Novae, Stellar Spectra, Infrared Spectra, Line Spectra, Radial Velocity

Scientific paper

About twenty spectra in a wide range up to 1.13 microns were obtained for the object identified as a nova in Scutum. The spectra are characterized by a strong continuum on which numerous large and intense emission lines are superimposed. Some lines are bordered by large absorption lines of complex structure. The following elements have been identified: H I, He I, C I, C II, N I, N II, N III, O I, O II, Mg II, and S I.

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