A new CH star in Omega Centauri

Details A new CH star in Omega Centauri A new CH star in Omega Centauri

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..835c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Sept. 1985, p. 835-837. NSF-supported research.

Astronomy and Astrophysics

Astronomy

8

Carbon Stars, Globular Clusters, Metallicity, Stellar Motions, Binary Stars, Cool Stars, Hot Stars, Iron, Radial Velocity, Stellar Magnitude

Scientific paper

ROA No. 577 is found to have the spectroscopic characteristics of the
Population II carbon stars known as CH stars. Its radial velocity and
proper motion show it to be a cluster member, although it is fainter
than the previously identified cool CH stars in ω Cen.

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