• DOI:10.1051/0004-6361/201423527
Corpus ID: 56077513

The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster gamma Velorum

@article{Spina2014TheGS,
  title={The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster gamma Velorum},
  author={L. Spina and S. Randich and F. Palla and G. Sacco and L. Magrini and E. Franciosini and L. Morbidelli and L. Prisinzano and E. J. Alfaro and K. Biazzo and A. Frasca and J. G. Hern'andez and S. Sousa and V. Adibekyan and E. Delgado-Mena and D. Montes and H. Tabernero and A. Klutsch and G. Gilmore and S. Feltzing and R. Jeffries and G. Micela and A. Vallenari and T. Bensby and A. Bragaglia and E. Flaccomio and S. Koposov and A. Lanzafame and E. Pancino and A. Recio-Blanco and R. Smiljanic and M. T. Costado and F. Damiani and V. Hill and A. Hourihane and P. Jofr'e and P. D. Laverny and T. Masseron and C. Worley},
  journal={Astronomy and Astrophysics},
  year={2014},
  volume={567}
}

L. Spina, S. Randich, +36 authors C. Worley

Published 2014

Physics

Astronomy and Astrophysics

Context. Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrichment by nearby supernova explosions to the ability to form planetary systems. In spite of this, detailed abundance studies are currently available for relatively few regions. Aims. In this context, we present the analysis of the metallicity of the Gamma Velorum cluster, based on the products distributed in… CONTINUE READING

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