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We present first results from the quantitative spectroscopic analysis of 266Galactic O-type stars targeted by the IACOB and OWN surveys (implying thelargest sample of stars of this type analyzed homogeneously). We also evaluatewhat is the present situation regarding available information about distances,as provided by the Hipparcos and Gaia missions.

Physical characterization of Galactic O-type stars targeted by the IACOB and OWN surveys