High-precision radial velocities for faint giants. I - MMT echelle results for globular cluster stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Giant Stars, Globular Clusters, Late Stars, Radial Velocity, Accuracy, Cross Correlation

Scientific paper

Velocities of accuracy 0.5 - 2.5 km s-1 are presented for 21 giants in eight nearby globular clusters, and for eight giants in four clusters located farther than 80 kpc from the galactic center. The measurements for the nearby cluster giants provide secondary velocity standards for cool metal-poor stars, while those of the remote giants allow more accurate cluster velocities to be derived.

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