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Fig. 11.

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Massive O and B stars from the recent catalogue of Pantaleoni González et al. (2021), superimposed on the dust extinction image in the horizontal plane containing the Sun. Only massive stars with identified stellar types, possessing EDR3 parallaxes, and located within 50 pc of the plane are represented. The colour scale and the size of the marker distinguish types from O3 (blue, large circles) to B9 (pink, small circles).

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