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- W1988848045 abstract "We use near-infrared observations of eight selected Galactic globular clusters to estimate their distances by comparing the observed and theoretically predicted K magnitudes of the red giant branch bumps and tips. The K magnitude levels of the RGB bump and tip have been measured from the luminosity function of the selected RGB stars in the clusters. Theoretical absolute <TEX>$M_k$</TEX> magnitudes of the RGB bump and tip are taken from the Yonsei-Yale isochrones. Comparing the observed apparent K magnitude with the derived absolute <TEX>$M_k$</TEX> magnitude, we calculate the distance moduli of the clusters. We discuss the dependency of the derived distance modulus on the cluster age and the uncertainty of the distance measurement from the near-infrared photometry of the RGB bump and tip." @default.
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- W1988848045 date "2006-06-01" @default.
- W1988848045 modified "2023-09-25" @default.
- W1988848045 title "RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: I. BUMP, TIP, AND DISTANCE FROM NEAR INERARED PHOTOMETRY" @default.
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- W1988848045 doi "https://doi.org/10.5140/jass.2006.23.2.091" @default.
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