Table A.3.
Expansion Velocities and kinematic Ages for a subsample of 65 PNe within GAPN-EDR3 sample.
PN Name | Radius | Velexp | Agekin |
---|---|---|---|
(pc) | (km/s) | (kyr) | |
Abell 24 | 0.687 | 14 | 32 |
Abell 28 | 0.302 | 4 | 49.3 |
Abell 29 | 1.17 | 25 | 30.5 |
Abell 3 | 0.344 | 30 | 7.5 |
Abell 31 | 1.202 | 29 | 27 |
Abell 33 | 0.653 | 32 | 13.3 |
Abell 34 | 0.826 | 35 | 15.4 |
Abell 39 | 0.455 | 29 | 10.2 |
Abell 51 | 0.252 | 42 | 3.9 |
Abell 61 | 0.789 | 32 | 16.1 |
Abell 7 | 0.972 | 29 | 21.9 |
Abell 71 | 0.426 | 20 | 13.9 |
Abell 74 | 1.307 | 27 | 31.6 |
Cn 3-1 | 0.07 | 10 | 4.6 |
H 2-1 | 0.026 | 36 | 0.5 |
HaWe 4 | 1.219 | 11 | 72.3 |
Hen 2-107 | 0.077 | 33 | 1.5 |
Hen 2-108 | 0.114 | 12 | 6.2 |
Hen 2-131 | 0.061 | 12 | 3.3 |
Hen 2-138 | 0.068 | 11 | 4 |
Hen 2-51 | 0.073 | 10 | 4.7 |
IC 1295 | 0.395 | 27 | 9.6 |
IC 2448 | 0.168 | 13.5 | 8.1 |
IC 289 | 0.167 | 25.5 | 4.3 |
IC 3568 | 0.092 | 8 | 7.5 |
IC 418 | 0.04 | 16 | 1.6 |
IC 4593 | 0.083 | 12 | 4.5 |
IC 4642 | 0.224 | 34.5 | 4.2 |
IC 5148/50 | 0.368 | 53 | 4.5 |
IsWe 2 | 1.711 | 8 | 139.5 |
Lo 1 | 0.813 | 30 | 17.7 |
M 1-26 | 0.041 | 12 | 2.2 |
M 1-46 | 0.063 | 7 | 5.9 |
M 1-53 | 0.072 | 13 | 3.6 |
M 1-65 | 0.054 | 4 | 8.9 |
M 1-77 | 0.05 | 6.5 | 5 |
M 2-33 | 0.049 | 12 | 2.6 |
M 3-34 | 0.071 | 14 | 3.3 |
NGC 2022 | 0.139 | 26 | 3.5 |
NGC 2792 | 0.108 | 20 | 3.5 |
NGC 3587 | 0.405 | 34 | 7.8 |
NGC 3699 | 0.147 | 27.5 | 3.5 |
NGC 4361 | 0.285 | 32 | 5.8 |
NGC 5882 | 0.069 | 11 | 4.1 |
NGC 6058 | 0.211 | 27 | 5.1 |
NGC 6072 | 0.178 | 6 | 19.3 |
NGC 6153 | 0.083 | 17 | 3.2 |
NGC 6210 | 0.065 | 21 | 2 |
NGC 6572 | 0.061 | 18 | 2.2 |
NGC 6772 | 0.184 | 11 | 10.9 |
NGC 6781 | 0.15 | 12 | 8.1 |
NGC 6842 | 0.281 | 35 | 5.2 |
NGC 6891 | 0.077 | 7 | 7.2 |
NGC 6894 | 0.203 | 43 | 3.1 |
NGC 7009 | 0.072 | 25 | 1.9 |
NGC 7094 | 0.393 | 45 | 5.7 |
NGC 7293 | 0.41 | 14 | 19.1 |
NGC 7354 | 0.164 | 25 | 4.3 |
NGC 7662 | 0.117 | 27 | 2.8 |
PuWe 1 | 1.156 | 23 | 32.8 |
Sh 2-216 | 1.835 | 4 | 299.3 |
Vy 2-3 | 0.055 | 12.5 | 2.9 |
We 1-10 | 1.1 | 26 | 27.6 |
WeDe 1 | 1.338 | 17 | 51.3 |
Wray 17-31 | 0.5 | 28 | 11.6 |
Notes. kinematic ages are calculated by multiplying the expansion velocities by a correction factor of 1.5, as proposed in Jacob et al. (2013). See Sect. 3.3 for more details.
References. Expansion velocities Velexp taken from Frew (2008) and Weinberger (1989).
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