Characterizing B stars from Kepler/K2 Campaign 11 - Optical analysis and seismic diagnostics

Open Access

Fig. E.12

ν versus $\sqrt{Δ v}$ $\sqrt {{\rm{\Delta }}v}$ diagram for EPIC 240353031. Frequencies between 7.3 and 22 μΗz were used, attributed to prograde sectoral modes with m = 1. For this star, we find that v_rot = 5.1 ± 0.1 μΗz, P₀ = 4.5 ± 0.3 · 10³ s.

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