Abstract
ABSTRACT The radial velocity of RGO 153, one of three carbon stars that have been found in the field of the globular cluster CL) Cen, differs by more than 250 km sec-1 from the mean cluster velocity, indicating that the star is not a physical member of the cluster. Key words: globular cluster - carbon star - radial velocity
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
More From: Publications of the Astronomical Society of the Pacific
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.