The Gaia-ESO survey: dynamical models of flattened, rotating globular clusters

We present a family of self-consistent axisymmetric rotating globular cluster models which are fitted to spectroscopic data for NGC 362, NGC 1851, NGC 2808, NGC 4372, NGC 5927 and NGC 6752 to provide constraints on their physical and kinematic properties, including their rotation signals. They are c...

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Bibliographic Details

Main Author:	Jeffreson, Sarah (Author)
Format:	Article (Journal)
Language:	English
Published:	11 May 2017
In:	Monthly notices of the Royal Astronomical Society Year: 2017, Volume: 469, Issue: 4, Pages: 4740-4762
ISSN:	1365-2966
DOI:	10.1093/mnras/stx1152
Online Access:	Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx1152
Author Notes:	S.M.R. Jeffreson, J.L. Sanders, N.W. Evans, A.A. Williams, G.F. Gilmore, A. Bayo, A. Bragaglia, A.R. Casey, E. Flaccomio, E. Franciosini, A. Hourihane, R.J. Jackson, R.D. Jeffries, P. Jofré, S. Koposov, C. Lardo, J. Lewis, L. Magrini, L. Morbidelli, E. Pancino, S. Randich, G.G. Sacco, C.C. Worley, S. Zaggia