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Bulgarian Chemical Communications
We probed to derive a new information on the massive star population and the extinction in the disc of Andormeda galaxy from a ground based UBV stellar photometry. Classical dereddening procedure was applied to evaluate both the extinction of starlight caused by the dust and the intrinsic properties (luminosity, color) of stars themselves. Thus, we were able draw conclusions about the spatial distribution of the dust, and-with the use of isocrones-to estimate the age of each successfullyfatcat:ed7ud6eydjdqfa3qyuoyfw3elm