Table 2
Parameters of the (new) hydrodynamical simulations used in this work.
| Sequence | Star/M⊙ | Mass loss | Velocity | Wind abund. | Neb. abund. |
|---|---|---|---|---|---|
| PN1 (a) | 0.595 | ṀPPKMH | VPPKMH | PN | PN |
| PN100 | 0.595 | ṀPPKMH × 100 | VPPKMH | PN | PN |
| PN100x5.5 | 0.595 | ṀppKMH × 100 | VPPKMH | PN | PN |
| WR1 | 0.595 | ṀppKMH | VPPKMH | WR | PN |
| WR3V05 | 0.595 | ṀPPKMH × 3 | VPPKMH/2 | WR | PN |
| WR10V05 | 0.595 | ṀPPKMH × 10 | VPPKMH/2 | WR | PN |
| WR10V05x2.0 | 0.595 | ṀPPKMH × 10 | VPPKMH/2 | WR | PN |
| WR10V05x0.25 | 0.595 | ṀppKMH × 10 | VPPKMH/2 | WR | PN |
| WR100 | 0.595 | ṀPPKMH × 100 | VPPKMH | WR | PN |
| WR100x5.5 | 0.595 | ṀppKMH × 100 | VPPKMH | WR | PN |
| WR100V05 | 0.595 | ṀPPKMH × 100 | VPPKMH/2 | WR | PN |
| WR100V05x5.5 | 0.595 | ṀPPKMH × 100 | VPPKMH/2 | WR | PN |
Notes. The sequences are labelled by the chemical composition of the post-AGB wind (‘PN’ or ‘WR’, Col. 5), followed by the mass-loss rate enhancement factor relative to the Pauldrach et al. (1988) prescription (cf. Col. 3), and the corresponding wind velocity factor (cf. Col. 4). The additions ‘…x2.0’ or ‘…x5.5’ mean that the evolution of the 0.595 M⊙ remnant is accelerated by a factor of 2 or 5.5, ‘…x0.25’ means a decelerated evolution by a factor of four. (a)Sequence 6a-HC2 of SSW but recalculated with the updated NEBEL code.
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