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The horizontal-branch stars in globular clusters. I - The period-shift effect, the luminosity of the horizontal branch, and the age-metallicity relation

Lee, Young-Wook, Demarque, Pierre, Zinn, Robert·1990·The Astrophysical Journal

Abstract

Synthetic models of the horizontal branches in globular clusters are constructed from a grid of the standard horizontal branch evolutionary tracks. The models are used to study the period shifts at constant T(eff) between RR Lyrae variables in globular clusters of different metallicities and the variation in horizontal-branch luminosity with the Fe/H ratio. The results suggest that the observed differences in the mean periods of the ab variables and the fraction of c-type variables between the two Oosterhoff groups are caused by a difference in the mean luminosity of the ab variables of about 0.18 bolometric mass and by the uneven distribution of variables across the instability strip in the group II clusters.

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Metadata

Authors
Lee, Y.-W., Demarque, P., & Zinn, R.
Venue
The Astrophysical Journal
Published
1990-02
Volume
350
Pages
155
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1988147641
Cited by
259
References
0
FWCI
10.42
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The horizontal-branch stars in globular clusters. I - The period-shift effect, the luminosity of the horizontal branch, and the age-metallicity relation. https://app.cochat.ai/papers/10.1086/168370
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Lee, Y.-W., Demarque, P., & Zinn, R. (1990). The horizontal-branch stars in globular clusters. I - The period-shift effect, the luminosity of the horizontal branch, and the age-metallicity relation. The Astrophysical Journal. https://doi.org/10.1086/168370

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