A new carbon-symbiotic star in the Large Magellanic Cloud
Journal Article
·
· Publications of the Astronomical Society of the Pacific; (USA)
- Arizona State Univ., Tempe (USA) Victoria Univ. (Canada)
A new carbon-symbiotic star, designated as CH-95, was discovered during a study of the kinematics of CH stars in the LMC. The spectrum of CH-95 is presented. Some of the strong emission lines found include H, He I, He II, forbidden O III, and the broad C III/N III blend at 4640 A, often seen in compact systems such as X-ray binaries. A comparison was made with other C-star symbiotics in the LMC, SMC, and Draco. 12 refs.
- OSTI ID:
- 7144165
- Journal Information:
- Publications of the Astronomical Society of the Pacific; (USA), Journal Name: Publications of the Astronomical Society of the Pacific; (USA) Vol. 101; ISSN PASPA; ISSN 0004-6280
- 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
CARBON STARS
COMPARATIVE EVALUATIONS
DETECTION
EMISSION SPECTRA
GALAXIES
MAGELLANIC CLOUDS
MAIN SEQUENCE STARS
SPECTRA
STARS
SYMBIOTIC STARS
VISIBLE SPECTRA
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CARBON STARS
COMPARATIVE EVALUATIONS
DETECTION
EMISSION SPECTRA
GALAXIES
MAGELLANIC CLOUDS
MAIN SEQUENCE STARS
SPECTRA
STARS
SYMBIOTIC STARS
VISIBLE SPECTRA