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Thanks to the high spatial resolution provided by long baselineinterferometry, it is possible to understand the complex circumstellar geometryaround stars with the B[e] phenomenon. These stars are composed by objects indifferent evolutionary stages, like high- and low-mass evolved stars,intermediate-mass pre-main sequence stars and symbiotic objects. However, up tonow more than 50% of the confirmed B[e] stars are not well classified, beingcalled unclassified B[e] stars. From instruments like VLTI/AMBER and VLTI/MIDI,we have identified the presence of gaseous and dusty circumstellar disks, whichhave provided us with some hints related to the nature of these objects. Here,we show our results for two galactic stars with the B[e] phenomenon, HD 50138and CPD-529243, based on interferometric measurements.

Stars with the B[e] phenomenon seen by long baseline interferometry