Shows low density structures
sketchfab
The Gaia DR2 catalog reveals a striking disparity between the actual and expected populations of stars within the upper main sequence. By meticulously analyzing the data, astronomers have pinpointed a significant drop-off in stellar density at approximately 6 solar masses. This trend is particularly pronounced when focusing on the region spanning from 5 to 10 solar masses. Furthermore, an examination of the Gaia DR2 data set also underscores the existence of a notable gap within this mass range.
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