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Table 2.

Comparison of the temperature regions to previously calculated pre-main-sequence instability strips.

MP98 G06 B11 G12 This work
Type Non-linear Linear Linear Linear Linear
Note TDC (a) TDC ASE (b)
Radial order 1–3 1–7 1–60 (c) ? 1–50
δ Sct 6500− 6450− 6300 (d)
7500 K 8400 K 10 300 K
γ Dor 6550− 5200−
7400 K 7650 K (e)
SPB 10 500− 11 100−
19 200 K 18 700 K

Notes.

(a)

Time dependent convection,

(b)

accretion from protostellar seed,

(c)

assumed from results,

(d)

the red edge of the p-mode instability region is taken to be the boundary to high normalised growth rates as discussed in the text.

(e)

The difference at the red edge is an accretion effect for modes with low radial order only. For radial orders ≥15, we obtain the temperature range 6450−7550 K.

References. MP98: Marconi & Palla (1998), G06: Grigahcene et al. (2006), B11: Bouabid et al. (2011), G12: Gruber et al. (2012).

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