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Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula. Methods. We investigate the properties of the two already known kinematic components (approaching and receding), which account for the ...


Damiani, F.Bonito, R.Magrini, L.Prisinzano, L.Mapelli, M.Micela, G.Kalari, V.Maíz Apellániz, J.Gilmore, G.Randich, S.Alfaro, E.Flaccomio, E.Koposov, S.Klutsch, A.Lanzafame, A. C.Pancino, E.Sacco, G. G.Bayo, A.Carraro, G.Casey, A. R.Costado, M. T.Franciosini, E.Hourihane, A.Lardo, C.Lewis, J.Monaco, L.Morbidelli, L.Worley, C.Zaggia, S.Zwitter, T.Dorda, R.[Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines]Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

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