Distributions and evolution of the equatorial rotation velocities of 2937 BAF-type main-sequence stars from asteroseismology - A break in the specific angular momentum at M ≃ 2.5 M⊙

Open Access

Fig. 4.

Histograms (upper panels) and KDEs (lower panels) of the near-core rotation frequency (left) and specific angular momentum (right), where the two samples are considered jointly, split up into five regimes of evolutionary stage from near-ZAMS (cyan) to near-TAMS (purple).

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