Fig. 12.

Kiel diagrams for models of NGC 6910-18. Leftmost panel: models that satisfy all criteria, (i) to (v), for the radial mode (f1). Black and blue dots correspond to modes with rotational velocities of 250 and 97 km s−1, respectively. The green area is the same as in Fig. 11; blue vertical lines correspond to the adopted Teff limits for NGC 6910-18. The models define three areas (shown with red boundaries) corresponding to f1 identified as fundamental (F), first overtone (1O), and second overtone (2O) radial mode. Remaining four panels: location of models satisfying all criteria for the f5 mode assuming (from left to right) l = 0, 1, 2, and 3. The colours of the dots have the same meaning as in the leftmost panel.
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