Hostname: page-component-7479d7b7d-c9gpj Total loading time: 0 Render date: 2024-07-11T05:02:57.187Z Has data issue: false hasContentIssue false
  • English
  • Français

Abundance ratios & ages of stellar populations in HARPS-GTO sample

Published online by Cambridge University Press:  07 March 2018

E. Delgado Mena Open the ORCID record for E. Delgado Mena [Opens in a new window] ,
M. Tsantaki ,
V. Zh. Adibekyan ,
S. G. Sousa ,
N. C. Santos ,
J. I. González Hernández  and
G. Israelian
E. Delgado Mena
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal. email: elisa.delgado@astro.up.pt
M. Tsantaki
Affiliation:
Instituto de Radioastronomía y Astrofísica, IRyA, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Michoacán, Mexico
V. Zh. Adibekyan
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal. email: elisa.delgado@astro.up.pt
S. G. Sousa
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal. email: elisa.delgado@astro.up.pt Departamento de Física e Astronomía, Faculdade de Ciências, U. Porto, Portugal
N. C. Santos
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal. email: elisa.delgado@astro.up.pt Departamento de Física e Astronomía, Faculdade de Ciências, U. Porto, Portugal
J. I. González Hernández
Affiliation:
Instituto de Astrofísica de Canarias, C/ Via Lactea, s/n, 38205, La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
G. Israelian
Affiliation:
Instituto de Astrofísica de Canarias, C/ Via Lactea, s/n, 38205, La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this work we present chemical abundances of heavy elements (Z>28) for a homogeneous sample of 1059 stars from HARPS planet search program. We also derive ages using parallaxes from Hipparcos and Gaia DR1 to compare the results. We study the [X/Fe] ratios for different populations and compare them with models of Galactic chemical evolution. We find that thick disk stars are chemically disjunt for Zn adn Eu. Moreover, the high-alpha metal-rich population presents an interesting behaviour, with clear overabundances of Cu and Zn and lower abundances of Y and Ba with respect to thin disk stars. Several abundance ratios present a significant correlation with age for chemically separated thin disk stars (regardless of their metallicity) but thick disk stars do not present that behaviour. Moreover, at supersolar metallicities the trends with age tend to be weaker for several elements.

Keywords

stars: abundancesstars: fundamental parametersGalaxy: evolutionGalaxy: disksolar neighborhood
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 156 - 159
Copyright
Copyright © International Astronomical Union 2018 

References

Adibekyan, V. Z., Santos, N. C., Sousa, S. G., & Israelian, G., 2011, A&A, 535, L11 Google Scholar
Adibekyan, V. Z., Sousa, S. G., Santos, N. C., et al., 2012, A&A, 545, A32 Google Scholar
Bertran de Lis, S., Delgado Mena, E., Adibekyan, V. Z., et al., 2015, A&A, 576, A89 Google Scholar
Bressan, A., Marigo, P., Girardi, L., et al., 2012, MNRAS, 427, 127 Google Scholar
da Silva, R., Porto de Mello, G. F., Milone, A. C., et al., 2012, A&A, 542, A84 Google Scholar
Delgado Mena, E., Bertrán de Lis, S., Adibekyan, V. Z., et al., 2015, A&A, 576, A69 Google Scholar
Delgado Mena, E., Israelian, G., González Hernández, J. I., et al., 2014, A&A, 562, A92 Google Scholar
Delgado Mena, E., Tsantaki, M., Adibekyan, V. Z., et al. 2017, arXiv:1705.04349 Google Scholar
Feltzing, S., Howes, L. M., & McMillan, P. J., Stonkutė, E., 2017, MNRAS, 465, L109 Google Scholar
Lindegren, L., Lammers, U., Bastian, U., et al., 2016, A&A, 595, A4 Google Scholar
Nissen, P. E., 2015, A&A, 579, A52 Google Scholar
Perryman, M. A. C., Lindegren, L., Kovalevsky, J., et al., 1997, A&A, 323, L49 Google Scholar
Spina, L., Meléndez, J., Karakas, A. I., et al., 2016, A&A, 593, A125 Google Scholar
Suárez-Andrés, L., Israelian, G., González Hernández, J. I., et al., 2016, A&A, 591, A69 Google Scholar
van Leeuwen, F., 2007, A&A, 474, 653 Google Scholar