Table 6
CSPNe wind terminal velocities.
| Name |
|
|
|
References |
| [km s-1] | [km s-1] | [km s-1] | ||
|
|
||||
| A 30 | 3000 | 3400 | 4000 | 1 |
| A 43 | 3000 | ... | ... | ... |
| A 78 | 3450 | 3500 | 3200 | 2 |
| BD+30°3639 | 670 | 1000 | 700 | 3 |
| Cn 3-1 | 380 | 330 | ... | 3 |
| Hb 7 | 1360: | 1320 | ... | 4 |
| Hen 2-99 | 870 | 1000–2000 | 900 | 5 |
| Hen 2-131 | 370 | 850 | 450 | 6 |
| Hen 2-138 | ... | ... | 300 | 7 |
| IC 418 | 450 | 1050 | 700 | 8 |
| IC 2149 | 930 | 1300 | 1000 | 8 |
| IC 2448 | 2280 | ... | 2000 | 9 |
| IC 2501 | 1210 | 1280 | ... | ... |
| IC 2553 | 2450 | ... | ... | ... |
| IC 3568 | 1580 | 1850 | 1730 | 10 |
| IC 4593 | 820 | 1100 | 750 | 9 |
| IC 4776 | 1840 | 1760 | 2300 | 2,6 |
| IC 5217 | 2360 | ... | ... | ... |
| K 1-16 | 3550: | 3800 | 4000 | 11,12 |
| Lo 4 | 3430: | ... | 4000 | 1,13 |
| LSS 1362 | 480 | ... | 2400 | ... |
| NGC 40 | 1030 | 1600 | 1000 | 3 |
| NGC 246 | 3390 | >3300 | 4000 | 11 |
| NGC 1535 | 1825: | 2150 | 1950 | 2 |
| NGC 2371-2 | 3500 | 4500 | 3700 | 2, 14 |
| NGC 2392 | 65 | 600 | 300 | 9 |
| NGC 2867 | 2110 | ... | 1800 | 1, 15 |
| NGC 5882 | 1720 | 1525 | ... | ... |
| NGC 6058 | 2600 | ... | 2300 | 9 |
| NGC 6210 | 2100 | 2350 | 2150 | 9 |
| NGC 6572 | 1140 | 1550 | 1190 | 10 |
| NGC 6543 | ... | ... | 1500 | 8 |
| NGC 6826 | 1100 | 1600 | 1200 | 6 |
| NGC 6891 | 950 | 1950 | ... | 16 |
| NGC 7009 | 2540 | 2750 | 2770 | 17,18 |
| NGC 7094 | 3610 | 3600 | 3500 | 11 |
| NGC 7662 | 1640: | ... | 2250 | 9 |
| PB 6 | 2980 | ... | 3000 | 1 |
| PB 8 | 1000 | 1060 | 1000 | 19 |
| RX J2117.1+3412 | 3140: | ... | 3500 | 11 |
| Sp 3 | 1680 | 1600 | ... | 4 |
| SwSt 1 | 880 | 1580 | 900 | 20 |
| Tc 1 | 1050 | 1530 | 900 | 6 |
| Vy 2-3 | 1460 | ... | ... | ... |
Notes.The “:” sign indicates that these velocities have been derived from P Cygni profiles that are not completely saturated.
Reference. (1) Koesterke (2001); (2) Herald & Bianchi (2004); (3) Marcolino et al. (2007a); (4) Gauba et al. (2001); (5) Leuenhagen et al. (1996); (6) Pauldrach et al. (2004); (7) Prinja et al. (2010); (8) Prinja et al. (2012b); (9) Herald & Bianchi (2011); (10) Modigliani et al. (1993); (11) Koesterke & Werner (1998); (12) Patriarchi & Perinotto (1996); (13) Feibelman (1999); (14) Feibelman (1997); (15) Feibelman (1998); (16) McCarthy et al. (1990); (17) Cerruti-Sola & Perinotto (1989); (18) Iping et al. (2006); (19) Todt et al. (2010); (20) De Marco et al. (2001).
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