Numerous blended Fe V, Fe VI emission lines identified in the ultraviolet spectrum of the WN 6 star HD 192163

Details Numerous blended Fe V, Fe VI emission lines identified in the ultraviolet spectrum of the WN 6 star HD 192163 Numerous blended Fe V, Fe VI emission lines identified in the ultraviolet spectrum of the WN 6 star HD 192163

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..455n&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, June 1985, p. 455-457) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

1

Emission Spectra, Iron, Line Spectra, Ultraviolet Spectra, Wolf-Rayet Stars, Abundance, Computerized Simulation, Helium, Spectrum Analysis

Scientific paper

From the study of a high-resolution spectrum of the WN6 star HD 192163 observed by means of the IUE satellite it has been concluded that most of the previously unidentified spectral features in the region 1245 - 1720 Å are due to the overlapping of pure or of P Cygni-type emission lines of Fe V and Fe VI. The estimated Fe/He ratio is found to be close to the solar value.

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