The far UV spectrum of the O4V(f) star 9 Sagittarii

Details The far UV spectrum of the O4V(f) star 9 Sagittarii The far UV spectrum of the O4V(f) star 9 Sagittarii

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179...13l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 1, May 1991, p. 13-37.

Astronomy and Astrophysics

Astrophysics

2

Far Ultraviolet Radiation, O Stars, Stellar Spectra, Ultraviolet Spectra, Iue, Radial Velocity, Resonance Lines

Scientific paper

A detailed list of line identifications of the far UV spectrum of the O4V(f) star 9 Sagittarii (HD 164794) in the wavelength range 1174-2000 A is presented. The identification is based on two spectra recorded in 1981 (on April 16 - SWP 13729 and on August 24 - SWP 14805) by the International Ultraviolet Explorer (IUE). In the list many unclassified lines are included. The radial velocities of all lines, classified and unclassified, are measured for both spectra and the mean velocities for different ions are discussed.

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