Stellar rotation periods from K2 Campaigns 0–18 - Evidence for rotation period bimodality and simultaneous variability decrease

Timo Reinhold; Saskia Hekker

doi:10.1051/0004-6361/201936887

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Volume 635 (March 2020)

A&A, 635 (2020) A43

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Fig. 6.

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Rotation periods versus effective temperature of all stars with peak heights h_peak > 0.5. The color-coding and isochrones are the same as in Fig. 5. The black diamonds show periods where a local minimum in the variability range was detected (see Fig. 7 and Sect. 4.2).

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