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Table 3
Illustration of the midplane and effective temperature for the models with 0.8 and 1.2 M⊙.
Midplane temperature Tc | |||
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|||
peak [K] | |||
M∗ [M⊙] | Ω∗ [ΩK] | BL | disk |
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|||
0.8 | 0.0 | 640 000 | 520 000 |
0.2 | 590 000 | 520 000 | |
0.4 | 520 000 | 520 000 | |
0.6 | 450 000 | 520 000 | |
0.8 | no peak | 520 000 | |
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|||
1.2 | 0.0 | 1 140 000 | 900 000 |
0.2 | 1 060 000 | 900 000 | |
0.4 | 950 000 | 900 000 | |
0.6 | 820 000 | 900 000 | |
0.8 | 650 000 | 900 000 | |
Effective temperature Teff | |||
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|||
peak [K] | |||
M∗ [M⊙] | Ω∗ [ΩK] | BL | disk |
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|||
0.8 | 0.0 | 400 000 | 64 000 |
0.2 | 360 000 | 64 000 | |
0.4 | 300 000 | 64 000 | |
0.6 | 235 000 | 64 000 | |
0.8 | 165 000 | 64 000 | |
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|||
1.2 | 0.0 | 690 000 | 125 000 |
0.2 | 625 000 | 125 000 | |
0.4 | 540 000 | 125 000 | |
0.6 | 440 000 | 125 000 | |
0.8 | 300 000 | 125 000 |
Notes. The table states the maximum temperatures both in the disk and in the BL for each stellar rotation rate.
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