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We present an analysis of the kinematic and morphological structure of thenebula around the LMC LBV candidate S 119. On HST images, we find apredominantly spherical nebula which, however, seems to be much better confinedin its eastern hemisphere than in the western one. The filamentary western partof the nebula is indicative of matter flowing out of the nebula's main body.This outflow is even more evidenced by our long-slit echelle spectra. They showthat, while most of the nebula has an expansion velocity of 25.5 km/s, theoutflowing material reaches velocities of almost 140 km/s, relative to thesystemic one. A ROSAT HRI image shows no trace of S 119 and thus no indicationsof hot or shocked material.

An outflow from the nebula around the LBV candidate S 119