A new carbon-symbiotic star in the Large Magellanic Cloud

Details A new carbon-symbiotic star in the Large Magellanic Cloud A new carbon-symbiotic star in the Large Magellanic Cloud

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..917c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Oct. 1989, p. 917-920. Research supported by NSF a

Other

6

Carbon Stars, Magellanic Clouds, Stellar Spectra, Symbiotic Stars, Emission Spectra, Late Stars, Visible Spectrum

Scientific paper

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.

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