Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T17:30:55.168Z Has data issue: false hasContentIssue false
  • English
  • Français

Abundances of seven red giants in the open cluster NGC 3114†

Published online by Cambridge University Press:  18 January 2010

C. B. Pereira  and
C. Quireza
C. B. Pereira
Affiliation:
Observatório Nacional, Rua General José Cristino 77, 20921-400 São Cristóvão, Rio de Janeiro, RJ Brazil email: [email protected], [email protected]
C. Quireza
Affiliation:
Observatório Nacional, Rua General José Cristino 77, 20921-400 São Cristóvão, Rio de Janeiro, RJ Brazil email: [email protected], [email protected]
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.

We present a chemical analysis of seven red giants in the open cluster NGC 3114. Our main goal is to investigate the chemical composition of this cluster, which is not yet available in the literature. We employed the FEROS spectrograph on the ESO 2.2m telescope. Atmospheric parameters and metallicity were derived from the measured equivalent widths of several iron lines using the spectral code moog and Kurucz model atmospheres. We obtained the abundances of O, Al, Ca, Mg, Si, Ti, Ni, Cr, Sc, Y, Zr, La, Ce and Nd by measuring the equivalent widths of the absorption lines of these elements. A mean metallicity of [Fe/H] = 0.05 ± 0.13 relative to the Sun was determined from the data of the red-giant members. This result is in good agreement with the Galactic-disk radial distribution of iron traced by open clusters. We did not find any intrinsic star-to-star scatter in the [element/Fe] ratios for the stars in this cluster. We compare our results with investigations of other open clusters. An age of 8.2 Gyr is derived from isochrone fits.

Keywords

open clusters and associations: individual (NGC 3114)Galaxy: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 495 - 498
Copyright
Copyright © International Astronomical Union 2010

References

Alonso, A., Arribas, S., & Martínez–Roger, C. 1999, A&AS, 140, 261Google Scholar
Bertelli, G., Bressan, A., Chiosi, C., Fagotto, F., & Nasi, E. 1994, A&AS, 106, 275Google Scholar
Carraro, G. & Patat, F. 2001, A&A, 379, 136Google Scholar
Clariá, J. J., Lapasset, E., & Minniti, D. 1989, A&AS, 78, 363Google Scholar
Feinstein, A. 1995, Rev. Mex. A&A, 2, 57Google Scholar
González, J. F. & Lapasset, E. 2001, AJ, 121, 2657CrossRefGoogle Scholar
Jankowitz, N. E. & McCosh, C. J. 1963, MNSSA, 22, 18Google Scholar
Junqueira, S. & Pereira, C. B., 2001, AJ, 122, 360CrossRefGoogle Scholar
Kaufer, A., Stahl, O., Tubbesing, S., Nørregaard, P., Avila, G., Francois, P., Pasquini, L., & Pizzella, A. 1999, ESO Messenger, 95, 8Google Scholar
Mermilliod, J. C., Mayor, M., & Udry, S. 2008, A&A, 485, 303Google Scholar
Paunzen, E., Pintado, O. I., & Maitzen, H. M. 2003, A&A, 412, 721Google Scholar
Pereira, C. B. 2005, AJ, 129, 2469CrossRefGoogle Scholar
Pereira, C. B. & Roig, F. 2009, AJ, 137, 118CrossRefGoogle Scholar
Sagar, R. & Sharples, R. M. 1991, A&AS, 88, 47Google Scholar
Schneider, H. & Weiss, W. W. 1988, A&AS, 75, 353Google Scholar
Sestito, P., Bragaglia, A., Randich, S., Pallavicini, R., Andrievsky, S. M., & Korotin, S. A. 2008, A&A, 488, 943Google Scholar