The Astrophysical Journal (Jan 2025)

Dependence of Multiband Absolute Magnitudes and Color Indexes of the Tip of the Red Giant Branch Stars on Metallicity in Galactic Globular Clusters

  • Zhenzhen Shao,
  • Shu Wang,
  • Biwei Jiang,
  • Xiaofeng Wang,
  • Zhishuai Ge,
  • Haichang Zhu

DOI
https://doi.org/10.3847/1538-4357/adae8e
Journal volume & issue
Vol. 980, no. 2
p. 218

Abstract

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The tip of the red giant branch (TRGB) stars have attracted intensive attention in recent years because their I -band absolute magnitudes, M _I , are often used for distance calibration in the Hubble constant measurements because of its almost independence on metallicity ([Fe/H]). However, a discrepancy exists between various studies, and the theoretical stellar model predicts the dependence of their luminosity on [Fe/H]. Here, we present a careful study of the dependence of absolute magnitudes and color indexes on metallicity in optical and near-infrared bands. With the TRGB stars identified in 33 Galactic globular clusters by the reddest color in the G _BP − G _RP versus G _RP diagram, it is confirmed that M _I is almost constant of −4.017 ± 0.036 ± 0.027 mag when [Fe/H] −1.2, M _I is found to become fainter with lower metallicity, which would lead to a larger Hubble constant. In the optical G _BP , G _RP , and V bands, the absolute magnitude of TRGB stars tends to increase with metallicity, while in the infrared J , H , and K _s bands, the variation with metallicity shows an inverse tendency. In addition, the analytical relations of the color indexes with metallicity are presented, which have smaller dispersion than those derived for the corresponding absolute magnitudes.

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