OCCASO III. Iron peak and $\alpha$ elements of 18 open clusters. Comparison with chemical evolution models and field stars
Abstract
The study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended abundance analysis of 10 species (Fe, Ni, Cr, V, Sc, Si, Ca, Ti, Mg, O) for red giant stars in 18 OCCASO clusters. This represents a homogeneous sample regarding the instrument features, method, line list and solar abundances from confirmed member stars. We perform an extensive comparison with previous results in the literature, and in particular with the Gaia FGK Benchmark stars Arcturus and $\mu$Leo. We investigate the dependence of [X/Fe] with metallicity, Galactocentric radius ($6.5
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Submitted on : Tuesday, September 17, 2019-8:09:01 AM
Last modification on : Tuesday, October 17, 2023-4:44:03 PM
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Identifiers
- HAL Id : hal-02289644 , version 1
- ARXIV : 1909.05865
- BIBCODE : 2019MNRAS.490.1821C
- DOI : 10.1093/mnras/stz2595
Cite
L. Casamiquela, S. Blanco-Cuaresma, R. Carrera, L. Balaguer-Nunez, C. Jordi, et al.. OCCASO III. Iron peak and $\alpha$ elements of 18 open clusters. Comparison with chemical evolution models and field stars. Monthly Notices of the Royal Astronomical Society, 2019, 490 (2), pp.1821-1842. ⟨10.1093/mnras/stz2595⟩. ⟨hal-02289644⟩
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