Fig. 14.
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P-mode instability regions dependent on the excited orders. The black lines show the accreting evolutionary track (dashed) and the pre-main-sequence evolution from this models (thin). Different coloured areas show the regions where modes with radial orders higher than n ≥ 1, 5, 15, and 25 are unstable. The colour code of the shown pulsators is the same as in Fig. 1.
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