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Using open clusters as tracers of the galactic disk history

Published online by Cambridge University Press:  02 August 2018

Orlando J. Katime Santrich ,
Silvia Rossi ,
Yuri Abuchaim  and
Geraldo Gonçalves
Orlando J. Katime Santrich
Affiliation:
Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, São Paulo, SP, Brazil. email: ojksantrich@usp.br
Silvia Rossi
Affiliation:
Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, São Paulo, SP, Brazil. email: ojksantrich@usp.br
Yuri Abuchaim
Affiliation:
Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, São Paulo, SP, Brazil. email: ojksantrich@usp.br
Geraldo Gonçalves
Affiliation:
Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, São Paulo, SP, Brazil. email: ojksantrich@usp.br
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Abstract

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Open clusters are important objects to study the galactic structure and its dynamical behavior as well as the stellar formation and evolution. We carried out a spectroscopic analysis to derive atmospheric parameters and chemical composition for 52 giant stars within 9 galactic open clusters. We have used the high-resolution spectra from FEROS, HARPS and UVES in the ESO archive. The methodology used is based on LTE-hypothesis. Abundances of C, N, O, Na, Mg, Al, Si, Ca, Ti, Cr, Ni, YII, LaII, CeII, and NdII were calculated. Although most of these clusters present spectroscopic analysis in the literature, some CNO and s-process abundances were not previously estimated or were calculated with high uncertainties. Several lines of such elements were identified and used to calculate new abundances and improve some previous one.

Keywords

stars: abundancesopen clusters and associations: generalstars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 312 - 313
Copyright
Copyright © International Astronomical Union 2018 

References

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