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Table 4
Comparison of the increase of mass-loss rates over the bi-stability jump(s) in the non-rotating Galactic Ekström et al. (2012) and Brott et al. (2011) evolutionary grids.
| Geneva | Bonn | |||||
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| M [M⊙] | Tjump1 [kK] |  (1) |
Tjump2 [kK] | (2) |
Tjump1 [kK] | (1) |
| 20 | 23.5 | 19.6 | 15.7–12.9 | 11.9 | 26.0–20.5 | 16.6 |
| 25 | 24.0 | 17.9 | 14.6–10.4 | 10.2 | 26.3–21.5 | 15.7 |
| 30 | – | – | – | – | 26.6–21.7 | 12.1 |
| 32 | 24.3 | 16.6 | 15.7 | 13.3 | – | – |
| 35 | – | – | – | – | 26.9–21.8 | 11.2 |
| 40 | 24.9 | 15.4 | 16.8 | 13.1 | 27.2–22.3 | 10.7 |
| 50 | 25.1 | 14.0 | 17.8 | 13.2 | 27.6–22.7 | 10.0 |
| 60 | 25.4 | 13.1 | 18.1 | 12.6 | 27.9–23.1 | 9.6 |
| average | 16.5 | 12.2 | 12.3 | |||
Notes. Ratios of Ṁ on the cool and hot side (i.e., below and above the jump temperature) exceed a factor of 10. Rotating models show similar ratios.
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