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The alpha-enhanced isochrones and their impact on the FITS to the Galactic globular cluster system

Salaris, Maurizio, Chieffi, Alessandro, Straniero, Oscar·1993·The Astrophysical Journal

Abstract

The effect produced by the enhancement of the alpha-elements O, Ne, Mg, Si, S, and Ca on the evolutionary properties of low-mass, low-metallicity stars is analyzed, with emphasis on the evolutionary phases which extend from the main sequence up to the H reignition on the AGB. It is found that evolutionary models (suitable for Population II stars) with alpha-enhanced chemical composition can be computed even though proper low-temperature opacities are not yet available, since it is demonstrated that most of the evolutionary properties of Population II stellar models are not influenced by the metal content included in the opacity coefficient below 12,000 K. The fit to Groombridge 1830 is discussed, and it is concluded that it is unnecessary, at present, to revise the value of the mixing-length parameter obtained by fitting the sun.

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Metadata

Authors
Salaris, M., Chieffi, A., & Straniero, O.
Venue
The Astrophysical Journal
Published
1993-09
Volume
414
Pages
580
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1989442665
Cited by
539
References
0
FWCI
5.99
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The alpha-enhanced isochrones and their impact on the FITS to the Galactic globular cluster system. https://app.cochat.ai/papers/10.1086/173105
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Salaris, M., Chieffi, A., & Straniero, O. (1993). The alpha-enhanced isochrones and their impact on the FITS to the Galactic globular cluster system. The Astrophysical Journal. https://doi.org/10.1086/173105

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