High-resolution abundance analysis of four red giants in the globular cluster NGC 6558
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Fecha
2018-11
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Facultad/escuela
Idioma
en
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Editor
EDP Sciences
Nombre de Curso
Licencia CC
Licencia CC
Resumen
Context. NGC 6558 is a bulge globular cluster with a blue horizontal branch (BHB), combined with a metallicity of [Fe/H] â‰-1.0. It is similar to HP 1 and NGC 6522, which could be among the oldest objects in the Galaxy. Element abundances in these clusters could reveal the nature of the first supernovae. Aims. We aim to carry out detailed spectroscopic analysis for four red giants of NGC 6558, in order to derive the abundances of the light elements C, N, O, Na, Al, the α-elements Mg, Si, Ca, Ti, and the heavy elements Y, Ba, and Eu. Methods. High-resolution spectra of four stars with FLAMES-UVES at VLT UT2-Kueyen were analysed. Spectroscopic parameter-derivation was based on excitation and ionization equilibrium of Feâraquo; I and Feâ» II. Results. This analysis results in a metallicity of [Fe/H] =-1.17 ± 0.10 for NGC 6558. We find the expected α-element enhancements in O and Mg with [O/Fe] = +0.40, [Mg/Fe] = +0.33, and low enhancements in Si and Ca. Ti has a moderate enhancement of [Ti/Fe] = +0.22. The r-element Eu appears very enhanced with a mean value of [Eu/Fe] = +0.63. The first peak s-elements Y and Sr are also enhanced, these results have however to be treated with caution, given the uncertainties in the continuum definition; the use of neutral species (Srâraquo; I, Yâ» I), instead of the dominant ionized species is another source of uncertainty. Ba appears to have a solar abundance ratio relative to Fe. Conclusions. NGC 6558 shows an abundance pattern that could be typical of the oldest inner bulge globular clusters, together with the pattern in the similar clusters NGC 6522 and HP 1. They show low abundances of the odd-Z elements Na and Al, and of the explosive nucleosynthesis α-elements Si, Ca, and Ti. The hydrostatic burning α-elements O and Mg are normally enhanced as expected in old stars enriched with yields from core-collapse supernovae, and the iron-peak elements Mn, Cu, Zn show low abundances, which is expected for Mn and Cu, but not for Zn. Finally, the cluster trio NGC 6558, NGC 6522, and HP 1 have relatively high abundances of first-peak heavy elements, variable second-peak element Ba, and the r-element Eu is enhanced. The latter is particularly high in NGC 6558. © 2018 ESO.
Notas
Indexación: Scopus.
A knowledgements. B.B. and E.B. acknowledge grants from CNPq, CAPES – Finance code 001, and Fapesp. L.M. and H.E. acknowledge CNPq/PIBIC fellowships. L.K. acknowledges a CNPq postdoctoral fellowship and the Fapesp grant 2016/24814-5. A.P.V. acknowledges the Fapesp postdoctoral fellowship no. 2017/15893-1. We thank Elvis Cantelli for data reduction. S.O. acknowledges the Dipartimento di Fisica e Astronomia dell’Università di Padova.
A knowledgements. B.B. and E.B. acknowledge grants from CNPq, CAPES – Finance code 001, and Fapesp. L.M. and H.E. acknowledge CNPq/PIBIC fellowships. L.K. acknowledges a CNPq postdoctoral fellowship and the Fapesp grant 2016/24814-5. A.P.V. acknowledges the Fapesp postdoctoral fellowship no. 2017/15893-1. We thank Elvis Cantelli for data reduction. S.O. acknowledges the Dipartimento di Fisica e Astronomia dell’Università di Padova.
Palabras clave
Galaxy: Bulge, Globular clusters: Individual: NGC 6558, Stars: Abundances
Citación
Astronomy and Astrophysics, 619, art. no. A178.