In the open cluster NGC 6067, fast-rotating eMSTO stars are redder and more centrally concentrated than slow rotators, which supports pre-main-sequence star-disk interactions as the origin of the extended main-sequence turn-off.
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The impact of stellar rotations and binaries on the shape of upper main sequence near turn off in open cluster NGC\,6067
In the open cluster NGC 6067, fast-rotating eMSTO stars are redder and more centrally concentrated than slow rotators, which supports pre-main-sequence star-disk interactions as the origin of the extended main-sequence turn-off.