G Aguaya Poster

Preliminary Results of Be Stars Proportion in LMC Open Clusters and Application to the NGC 1850 Star Formation Region
G. Aguayo (ESO/Universidad de Concepcion), H. Garrido, C. Martayan, D. Baade, T. Rivinius, S. Stefl, and R. Mennickent

Using the ESO Wide Field Imager in its slitless spectroscopic mode, we report on the preliminary results of the Be stars proportion in various LMC open clusters compared to the SMC and the Galaxy.We also report on the populations of emission-line stars found in the LMC cluster NGC1850 and its vicinity. Those results combined to some photometric data show a possible spatial and mass segregation of the various populations of ELS, probably related to the star formation history on this region of the LMC.