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Fig. 14

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Position of the pulsating stars in the Kiel (top) and HRD (bottom) diagram. The different types of pulsators are indicated with various symbols: rapid pulsators sdBVr (open red circles), slow pulsators sdBVs (open blue circles), and hybrid pulsators sdBVrs (green filled circles). Stars found to be constant are indicated with grey filled circles. Feige 46 and LSIV-14°116 (blue open squares) are peculiar slow pulsators belonging to the small class of iHe-sdOBV (V366 Aqr). The ZAEHB (dashed line) is indicated for a core mass of 0.47 M and corresponding evolutionary sequences of the core-helium burning phase are shown for different H-envelope masses (dotted lines). Stars with a poor parallax measurement are excluded in the bottom panel. Representative errors are shown in each panel.

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