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26 April 2024
 
  » arxiv » 1501.1330

 Article overview



The Gaia-ESO Survey: Discovery of a spatially extended low-mass population in the Vela OB2 association
G.G. Sacco ; R.D. Jeffries ; S. Randich ; E. Franciosini ; R.J. Jackson ; M. Cottaar ; L. Spina ; F. Palla ; M. Mapelli ; E.J. Alfaro ; R. Bonito ; F. Damiani ; A. Frasca ; A. Klutsch ; A. Lanzafame ; A. Bayo ; D. Barrado ; F. Jimenez-Esteban ; G. Gilmore ; G. Micela ; A. Vallenari ; C. Allende Prieto ; E. Flaccomio ; G. Carraro ; M.T. Costado ; P. Jofre ; C. Lardo ; L. Magrini ; L. Morbidelli ; L. Prisinzano ; L. Sbordone ;
Date 6 Jan 2015
AbstractThe nearby (distance~350-400 pc), rich Vela OB2 association, includes $gamma^2$ Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for investigating the formation and early evolution of young clusters. Recent Gaia-ESO survey observations have led to the discovery of two kinematically distinct populations in the young (10-15 Myr) cluster immediately surrounding $gamma^2$ Velorum. Here we analyse the results of Gaia-ESO survey observations of NGC 2547, a 35 Myr cluster located two degrees south of $gamma^2$ Velorum. The radial velocity distribution of lithium-rich pre-main sequence stars shows a secondary population that is kinematically distinct from and younger than NGC 2547. The radial velocities, lithium absorption lines, and the positions in a colour-magnitude diagram of this secondary population are consistent with those of one of the components discovered around $gamma^2$ Velorum. This result shows that there is a young, low-mass stellar population spread over at least several square degrees in the Vela OB2 association. This population could have originally been part of a cluster around $gamma^2$ Velorum that expanded after gas expulsion or formed in a less dense environment that is spread over the whole Vela OB2 region.
Source arXiv, 1501.1330
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