The Gaia-ESO Survey: evidence of atomic diffusion in M67?

ABSTRACT. Investigating the chemical homogeneity of stars born from the same molecular cloud at virtually the same time is very important for our understanding

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Bibliographic Details
Main Authors: Bertelli Motta, Clio (Author) , Pasquali, Anna (Author) , Grebel, Eva K. (Author)
Format: Article (Journal)
Language:English
Published: 2018 March 14
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 478, Issue: 1, Pages: 425-438
ISSN:1365-2966
DOI:10.1093/mnras/sty1011
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1011
Verlag, Volltext: https://academic.oup.com/mnras/article/478/1/425/4983131
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Author Notes:C. Bertelli Motta, A. Pasquali, J. Richer, G. Michaud, M. Salaris, A. Bragaglia, L. Magrini, S. Randich, E.K. Grebel, V. Adibekyan, S. Blanco-Cuaresma, A. Drazdauskas, X. Fu, S. Martell, G. Tautvaišienė, G. Gilmore, E.J. Alfaro, T. Bensby, E. Flaccomio, S.E. Koposov, A.J. Korn, A.C. Lanzafame, R. Smiljanic, A. Bayo, G. Carraro, A.R. Casey, M.T. Costado, F. Damiani, E. Franciosini, U. Heiter, A. Hourihane, P. Jofré, C. Lardo, J. Lewis, L. Monaco, L. Morbidelli, G.G. Sacco, S.G. Sousa, C.C. Worley and S. Zaggia
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Summary:ABSTRACT. Investigating the chemical homogeneity of stars born from the same molecular cloud at virtually the same time is very important for our understanding
Item Description:Gesehen am 05.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty1011