Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

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

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6175961
Simulation analysis of a high-resolution IUE spectrum of the WN 6 star HD 192163 shows that most of the hitherto unidentified features at lambda = 1245--1720 A represent overlapping Fe V and Fe VI lines (pure emission or P Cygni profiles). A near-solar (Fe/He) abundance ratio is obtained.
Research Organization:
Institute of Astrophysics and Atmospheric Physics, Estonian Academy of Sciences, Tartu
OSTI ID:
6175961
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 11:3; ISSN SALED
Country of Publication:
United States
Language:
English

Similar Records

Profile of He I lambda5876 in the P-Cygni-type of star HD 152408
Journal Article · Wed Oct 01 00:00:00 EDT 1975 · Publ. Astron. Soc. Pac., v. 87, no. 519, pp. 735-736 · OSTI ID:4086177

Infrared spectra of the WN stars HD 50896 and HD 151932
Journal Article · Fri Dec 31 23:00:00 EST 1976 · Publ. Astron. Soc. Pac.; (United States) · OSTI ID:5299366

HD 192163, a possible Wolf-Rayet binary with a relativistic component
Journal Article · Wed Jul 01 00:00:00 EDT 1981 · Sov. Astron. Lett. (Engl. Transl.); (United States) · OSTI ID:5568733