Cited by 64Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchGalaxies: Formation, Evolution, Phenomena

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The 'Red Giant Clock' as an indicator for the efficiency of central mixing in horizontal-branch stars

Caputo, F., Chieffi, A., Tornambe, A., Castellani, V., Pulone, L.·1989·The Astrophysical Journal

Abstract

New evolutionary evaluations have been compared with observational data for the globular cluster M5 in order to assess the kind of mixing (semiconvection with and without the inclusion of the breathing pulses or overshooting) which takes place in real stars during the central He-burning phase. It is suggested that the evolutionary time scale on the red giant branch should be used to assess the absolute time scale of evolution on the asymptotic giant branch. On this basis, it is found that ordinary semiconvection without breathing pulses leads to the best match to the observed data for M5.

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Crossref · 10.1086/167387

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Metadata

Authors
Caputo, F., Chieffi, A., Tornambe, A., Castellani, V., & Pulone, L.
Venue
The Astrophysical Journal
Published
1989-05
Volume
340
Pages
241
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1980695895
Cited by
64
References
0
Citations by year
2026: 1 · 2025: 3 · 2024: 4 · 2023: 1 · 2022: 2 · 2021: 2 · 2020: 1 · 2018: 6 · 2017: 3 · 2016: 6 · 2015: 3 · 2014: 2 · 2013: 1 · 2012: 1
FWCI
0.00
Type
journal article
Language
en
Open access
closed
Locations
The Astrophysical Journal (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
red giant branch, semiconvection, overshoot, horizontal branch stars, asymptotic giant branch, helium burning

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