The Composition of Horizontal Branch Stars in the Globular Cluster Messier 10

Details The Composition of Horizontal Branch Stars in the Globular Cluster Messier 10 The Composition of Horizontal Branch Stars in the Globular Cluster Messier 10

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110412b&link_type=abstract

American Astronomical Society, AAS Meeting #211, #104.12; Bulletin of the American Astronomical Society, Vol. 39, p.926

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Scientific paper

Moderate resolution spectra of horizontal branch and lower giant branch stars in the globular cluster Messier 10 (NGC 6254) are analyzed to determine their compositions. The spectra were obtained using the Hydra fiber positioner and Bench Spectrograph on the WIYN 3.5-m telescope. The compositions are determined using fine analysis, and the compositions of stars in M10 are compared to other globular clusters. Radial velocity is used to confirm membership of the stars in M10.
This material is based upon work supported by the National Science Foundation through an REU Site Program grant to Tennessee State University and Indiana University. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the authors and do not necessarily reflect the views of the National Science Foundation.

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