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
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
CHARGED PARTICLES
ELEMENT ABUNDANCE
ELEMENTS
FLUIDS
GASES
HELIUM
IONS
IRON IONS
MAIN SEQUENCE STARS
NONMETALS
RARE GASES
SPECTRA
STARS
TEMPERATURE MEASUREMENT
ULTRAVIOLET SPECTRA
WOLF-RAYET STARS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
CHARGED PARTICLES
ELEMENT ABUNDANCE
ELEMENTS
FLUIDS
GASES
HELIUM
IONS
IRON IONS
MAIN SEQUENCE STARS
NONMETALS
RARE GASES
SPECTRA
STARS
TEMPERATURE MEASUREMENT
ULTRAVIOLET SPECTRA
WOLF-RAYET STARS