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Table 1

The main parameters of the interacting planetary nebulae sample.

No. PN l b Ref. IA e D Method Ref. θ Ref. Vexp Ref. Z R Tdyn WZO
(pc) (′′) (km s-1) (pc) (pc) (yrs) stage

1 A 13 204.02 –8.52 1, 2 57 8 944 Ph02 76.5 1 21.3 1 140 0.35 1.61E+04 WZO2
2 A 15 233.53 –16.31 1 70 4 1460 Ph02 17 1 35 1 416 0.12 3.37E+03 WZO2
3 A 16 153.77 22.83 1, 2 55 5 1912 Ph02 52.5 1 20 762 0.49 2.38E+04 WZO2
4 A 19 200.79 8.45 1 78 8 2609 Ph02 33.5 1 20 385 0.42 2.07E+04 WZO2
5 A 21 205.14 14.24 3, 4, 5, 6 39 3 557 Ind 1, 2 307.5 1 45 2 138 0.83 1.81E+04 WZO3
6 A 30 208.56 33.29 7 1155 Ind 9, 10 63.5 1 40 1 671 0.36 8.70E+03 WZO2
7 A 31 219.13 31.29 4, 5, 9 41 4 779 Ind 2, 12 485 1 22.5 1 425 1.83 7.97E+04 WZO2
8 A 34 248.71 29.54 9 80 9 773 Ph02 145 1 34 1 399 0.54 1.57E+04 WZO2
9 A 35 303.57 40.00 4, 5, 6, 11 78 3 167 Ind 1, 4 385 1 4.07 1 117 0.31 7.51E+04 WZO4
10 A 36 318.46 41.50 1, 4 85 8 370 Ind 1, 3 185 1 35 1 268 0.33 9.28E+03 WZO2
11 A 45 20.20 –0.65 5 60 11 700 St 17 142.5 1 20 8 0.48 2.37E+04 WZO2
12 A 52 50.41 5.29 1, 2, 3 28 5 3407 Ph02 18.5 1 20 314 0.31 1.50E+04 WZO2
13 A 58 37.60 –5.16 1, 2, 6 75 8 4807 Ph02 20 1 20 433 0.47 2.28E+04 WZO2
14 A 59 53.40 3.06 2, 12 72 16 1247 Ph02 43.5 1 20 67 0.26 1.29E+04 WZO3
15 A 6 136.10 4.93 1 45 5 1203 Ph02 93 1 20 104 0.54 2.65E+04 WZO2
16 A 61 77.70 14.78 9 90 6 1380 Ind 12 100 1 30 1 356 0.67 2.18E+04 WZO2
17 A 62 47.18 –4.29 1, 13 37 20 302 Ph02 80.5 1 17 1, 2 23 0.12 6.78E+03 WZO2
18 A 71 85.00 4.49 1 41 11 2800 Ind 16 78.5 1 15 1 219 1.07 6.96E+04 WZO2
19 A 74 72.66 –17.15 4, 5, 6, 13 61 16 800 Ind 1, 2 415 1 26.5 1 239 1.61 5.95E+04 WZO3
20 A 75 101.86 8.75 1, 3 69 12 1421 Ph02 28 1 42 1 217 0.19 4.50E+03 WZO1
21 A 78 81.30 –14.91 1 7 1 1165 Ind 9, 10 53.5 1 25 3 303 0.30 1.18E+04 WZO2
22 A 86 118.79 8.24 1, 2 54 7 2186 Ph02 31.5 1 20 314 0.33 1.63E+04 WZO2
23 Ba 1 171.30 –25.81 2 63 12 2077 Ph02 19 1 35.5 1 936 0.19 5.28E+03 WZO1
24 CN 1-5 2.29 –9.48 1 51 12 1664 Ph02 3.5 1 18 1 275 0.03 1.54E+03 WZO1
25 DeHt 2 27.65 16.92 2 32 4 2380 Ind 12 47 1 20 703 0.54 2.66E+04 WZO1
26 DeHt 4 48.76 –1.53 1, 2 64 9 6284 Ph02 20 1 20 168 0.61 2.98E+04 WZO2
27 DHW 1-2 11.40 17.99 15 46 9 1883 Ph02 13.5 1 20 591 0.12 6.04E+03 WZO3
28 DHW 5 111.09 11.64 1, 3, 4, 5, 6 84 12 330 Ind 1 264 2 5 1 67 0.42 8.27E+04 WZO4
29 EGB 4 143.60 23.82 1, 2 45 14 611 Ph02 55.5 1 20 254 0.16 8.05E+03 WZO3
30 EGB 6 221.59 46.36 4, 5 84 2 525 Ind 1 360 1 38.5 1 425 0.92 2.33E+04 WZO2
31 EGB 9 209.43 9.50 16 83 5 343 Ph02 152.8 3 20 57 0.25 1.24E+04 WZO4
32 ESO 320-28 291.43 19.26 1 5 5 6000 Ind 15 16 1 20 2017 0.47 2.28E+04 WZO2
33 HaTr 1 299.49 –4.12 16, 17 30 10 5925 Ph02 36 1 20 426 1.03 5.06E+04 WZO2
34 HDW 1 124.06 10.72 1, 3 45 16 530 Ind 1 135 1 20 99 0.35 1.70E+04 WZO3
35 HDW 5 218.99 –10.78 1, 18, 19 72 19 1962 Ph02 47 1 20 369 0.45 2.19E+04 WZO3
36 HDW 6 192.53 7.22 1 70 14 2256 Ph02 38 1 20 284 0.42 2.03E+04 WZO4
37 He 2-428 49.41 2.48 1, 2, 19 49 4 950 Ind 1 4.8 1 15 4 41 0.02 1.44E+03 WZO2
38 HFG 1 136.38 5.55 4, 5, 13 47 2 409 Ph02 250 1 14 1 40 0.50 3.47E+04 WZO1
39 HW 4 149.50 –9.28 4, 5, 6 90 8 380 Ind 1, 12 270 1 20 62 0.50 2.44E+04 WZO3
40 IC 4593 25.33 40.84 2, 7, 20 43 3 1082 Ph02 6.5 1 12.3 1 771 0.03 2.73E+03 WZO1
41 IW 1 149.71 –3.40 4, 5, 6, 13 75 9 510 Ind 1, 12 390 1 8.50 1, 5 30 0.96 1.11E+05 WZO3
42 IW 2 107.73 7.81 4, 5, 6, 13 43 13 650 Ind 1 450 1 12 1 89 1.42 1.16E+05 WZO3
43 Jacoby 1 85.50 46.50 5, 21 75 2 1100 Ind 29 327 4 20 893 1.74 8.54E+04 WZO2
44 JaFu 2 353.52 –5.00 6 73 2 9100 Ind 24 2.5 5 WZO3
45 Jn 1 104.21 –29.64 1, 2 24 1 755 Ind 1, 19 160 1 15 1 413.9 0.621 4.05E+04 WZO3
46 K 1-27 286.88 –29.58 1 55 16 1200 Ind 1 23 1 20 619 0.13 6.55E+03 WZO2
47 K 1-28 270.17 24.84 1 86 17 27 1 20 WZO2
48 K 1-3 346.98 12.46 1 1596 Ph02 46 1 17 1 347 0.36 2.05E+04
49 K 1-6 107.05 21.39 22 45 14 760 St 33 108 6 20 284 0.40 1.95E+04 WZO3
50 K 2-2 204.15 4.73 1, 2, 4 79 7 630 Ind 12 207.5 1 10 1 52 0.63 6.21E+04 WZO3
51 K 4-5 26.65 –1.58 2 80 12 11477 Ph02 2.8 1 20 317 0.16 7.63E+03 WZO3
52 KeWe 3 238.42 –1.87 16, 23, 24 55 12 686 Ph02 120 3 20 22 0.40 1.95E+04 WZO3
53 KeWe 5 348.94 4.61 23 86 4 8000 St 25 7.5 7 20 644 0.29 1.42E+04 WZO2
54 KFR 1 296.38 3.14 25 60 17 47.5 8 WZO3
55 Lo 10 328.20 1.41 1 75 9 6 1 WZO2
56 LoTr 1 228.21 –22.14 4, 26 89 11 1500 St 30 66 1 20 580 0.48 2.35E+04 WZO3
57 M 1-46 16.45 –1.98 27 1300 Ind 5 5.5 1 7 1 45 0.03 4.85E+03 WZO1
58 M 2-2 147.87 4.20 1, 2 74 8 1595 Ph02 3.05 1 14.3 1 117 0.02 1.61E+03 WZO2
59 M 2-40 24.12 3.88 1, 2, 28, 29 53 5 2016 Ph02 2.5 1 18 6 137 0.02 1.33E+03 WZO1
60 M 2-44 28.60 1.66 1, 2 50 13 1520 Ph02 3.7 1 12 1 44 0.03 2.22E+03 WZO1
61 MA 3 23.02 4.31 28, 30 35 17 2.5 1 5 6 WZO1
62 MeWe 1-1 272.41 –5.97 16, 17, 24, 25 80 2 1170 Ind 18 55 1 20 122 0.31 1.53E+04 WZO3
63 MeWe 1-2 283.45 –1.39 16, 24 61 10 132 9 WZO4
64 MeWe 1-4 315.99 8.24 16, 17, 24 75 9 2170 Ph02 65.25 3 20 312 0.69 3.36E+04 WZO3
65 MeWe 2-4 314.09 10.68 16, 24 56 14 240 8 WZO3
66 MWP 1 80.36 –10.41 5 68 7 600 Ind 1 5.5 10 20 109 0.02 7.83E+02 WZO3
67 NeVe 3-1 275.89 –1.02 16, 23, 24 47 5 28.75 8 WZO3
68 NeVe 3-6 292.48 0.88 31 70 4 5000 Ind 20 19.75 8 20 77 0.48 2.34E+04 WZO3
69 NGC 1360 220.36 –53.93 1, 35 50 15 385 Ind 1, 3 192.5 1 28 1 362 0.36 1.26E+04 WZO2
70 NGC 2438 231.80 4.12 14, 23 63 9 2000 Ind 7 32 1 21.2 1 144 0.31 1.43E+04 WZO1
71 NGC 2440 234.84 2.42 23, 33 49 5 1753 Ind 21 8 1 22.5 1 74 0.07 2.96E+03 WZO1
72 NGC 246 118.86 –74.71 1, 4, 33, 34 74 8 450 Ind 1 122.5 1 39.5 1, 2 587 0.27 6.62E+03 WZO3
73 NGC 2867 278.16 –5.94 1 49 10 1900 Ind 21 7 1 21.2 1 197 0.06 2.98E+03 WZO1
74 NGC 2899 277.15 –3.83 36, 37, 38 78 2 687 Ph02 45 1 25 1 46 0.15 5.87E+03 WZO2
75 NGC 3242 261.05 32.05 1, 32, 35 76 13 420 Ind 1 12.5 1 22.5 1 235 0.03 1.11E+03 WZO1
76 NGC 3587 148.49 57.05 39, 40 67 3 550 Ind 1 85 1 37.67 1, 7 548 0.23 5.89E+03 WZO1
77 NGC 40 120.02 9.87 1, 8, 29 90 3 800 Ind 3, 8 24 1 26.33 1, 2 138 0.09 3.46E+03 WZO2
78 NGC 6578 10.82 –1.83 1, 27 34 6 2000 Ind 22 4.25 1 19.2 1 64 0.04 2.10E+03 WZO1
79 NGC 6629 9.41 –5.05 1, 27, 32, 33 53 4 1950 Ind 21 7.75 1 20.17 1, 8 172 0.07 3.56E+03 WZO1
80 NGC 6751 29.23 –5.94 41, 42 1961 Ind 21 10.25 1 39 1 203 0.10 2.45E+03 WZO1
81 NGC 6765 62.46 9.56 1, 2 45 6 1521 Ph02 20 1 35 1 254 0.15 4.13E+03 WZO1
82 NGC 6772 33.16 –6.39 32 77 12 1260 Ind 21 32 1 17.6 1 140 0.20 1.09E+04 WZO1
83 NGC 6781 41.84 –2.99 3 76 2 1567 Ind 21 54 1 18 1, 8 82 0.41 2.23E+04 WZO2
84 NGC 6804 45.75 –4.59 28 82 3 1525 Ind 21 17.5 1 24 1 122 0.13 5.28E+03 WZO1
85 NGC 6826 83.56 12.79 37, 38 45 4 1550 Ind 5, 8 12.5 1 11 1 346 0.09 8.36E+03 WZO1
86 NGC 6842 65.91 0.60 1, 3 85 3 2700 Ind 16 28.5 1 35 1 28 0.37 1.04E+04 WZO1
87 NGC 6853 60.84 –3.70 2, 4, 5 74 4 408 Ind 2, 11, 14 201 1 25.5 1 26 0.40 1.53E+04 WZO1
88 NGC 6891 54.20 –12.11 2 45 3 2800 Ind 5, 8 7.5 1 8.4 1, 8 592 0.10 1.19E+04 WZO1
89 NGC 6894 69.48 –2.62 1, 43 1000 Ind 16 20 1 43 1 46 0.10 2.21E+03 WZO1
90 NGC 7094 66.78 –28.20 1 57 3 1623 Ind 10, 12 47 1 45 1 799 0.37 8.05E+03 WZO2
91 NGC 7293 36.16 –57.12 1, 4, 5 45 2 218 Ind 2, 14 490 1 31 3 217 0.52 1.63E+04 WZO1
92 Pe 1-16 26.34 –2.28 1 62 9 6156 Ph02 3.8 1 20 245 0.11 5.55E+03 WZO2
93 PFP 1 222.13 3.91 44 10 4 334 Ph02 570 11 20 23 0.92 4.51E+04 WZO2
94 PG 1034+001 247.55 47.75 10 79 11 155 St 34 10800 12 20 129 8.12 3.97E+05 WZO4
95 PM 1-295 51.36 1.81 28 5 17 1700 St 27 10 1 17 6 54 0.08 4.75E+03 WZO1
96 PN in M 22 9.87 –7.56 4 57 5 2700 Ind 31, 32 4.25 1 20 356 0.06 2.72E+03 WZO3
97 PW 1 158.92 17.86 4, 5 76 8 333 Ind 1, 2 600 1 24.7 1, 2 104 0.97 3.84E+04 WZO2
98 RE 1738+665 96.89 31.96 5 76 13 190 Ind 1, 2 1800 13 20 106 1.66 8.12E+04 WZO4
99 S 174 120.22 18.43 5 52 15 540 Ind 1, 12 375 13 20 174 0.98 4.81E+04 WZO3
100 S 176 120.29 –5.40 4, 5, 13 82 4 630 Ind 1 360 1 19 1 59 1.10 5.67E+04 WZO3
101 S 188 128.05 –4.07 1, 2, 4, 5, 6, 13 47 8 650 Ind 1 170 1 40 1 46 0.54 1.31E+04 WZO3
102 S 200 138.13 4.12 4 25 9 580 St 26 170 14 13 1 42 0.48 3.60E+04 WZO1
103 S 216 158.49 0.47 4, 5, 33 62 5 130 Ind 1, 2 3000 13 7 5 1 1.89 2.64E+05 WZO3
104 S 68 30.67 6.28 5, 13, 33 75 14 700 Ind 1 200 1 6.6 9 77 0.68 1.01E+05 WZO4
105 S 78 46.83 3.84 5 84 17 1420 Ind 19 300 1 20 95 2.07 1.01E+05 WZO4
106 Sd 1 78.93 0.76 1, 2 16 3 1949 Ph02 3.8 1 20 26 0.04 1.76E+03 WZO2
107 Sn 1 13.32 32.74 3 57 9 11900 Ind 5 3 1 WZO3
108 SuWt 1 309.30 1.39 16 87 12 526 Ph02 34 1 20 13 0.09 4.25E+03 WZO3
109 Tc 1 345.24 –8.84 1, 16 87 15 2300 Ind 8 4.5 1 8 1, 2 355 0.05 6.14E+03 WZO1
110 Ton 320 191.40 33.08 5 39 6 350 Ind 1 900 13 20 1 202 1.53 7.48E+04 WZO3
111 Vy 2-3 107.60 –13.32 28 64 13 5185 Ph02 2.1 1 13.1 6 1206 0.05 3.95E+03 WZO1
112 WDHS 1 197.41 –6.44 4, 5 30 5 750 Ind 1 462.5 1 17 1, 5 84 1.68 9.69E+04 WZO3
113 We 1-5 216.31 –4.49 1 61 6 5716 Ph02 7.5 1 20 448 0.21 1.02E+04 WZO2
114 We 1-6 224.94 1.06 1 2 9 1100 Ind 13 31 1 20 20 0.17 8.09E+03 WZO2
115 WeSb 5 58.69 –5.58 3, 24 80 5 1200 St 28 75 1 20 117 0.44 2.14E+04 WZO3
116 Wray 17-18 262.65 –4.62 1 30 8 6846 Ph02 10 1 20 552 0.33 1.62E+04 WZO2
117 YM 16 38.71 1.97 6 56 6 500 St 17 152 1 20 17 0.37 1.80E+04 WZO3

Notes. References for interaction: (1) Soker (1997); (2) Wareing et al. (2007); (3) Rauch & Kerber (2005); (4) Borkowski et al. (1990); (5) Tweedy & Kwitter (1996); (6) Dgani & Soker (1998); (7) Soker (1999); (8) Ramos-Larios et al. (2011); (9) Tweedy & Kwitter (1994a); (10) Rauch et al. (2004); (11) Jacoby (1981); (12) Kwitter et al. (1988); (13) Xilouris et al. (1996); (14) Pierce et al. (2004); (15) Kerber et al. (1997); (16) Kerber et al. (2000a); (17) Kerber (1998); (18) Ali & Pfleiderer (1999); (19) Soker & Hadar (2002); Zucker & Soker (1993); (21) Jacoby & Van de Steene (1995); (22) Frew et al. (2011); (23) Kerber et al. (1998); (24) Ali et al. (2000); (25) Rauch et al. (2000); (26) Bond & Livio (1990); (27) Corradi et al. (2003); (28) Guerrero et al. (1998); (29) Martin et al. (2002); (30) Villaver et al. (2003); (31) Kerber et al. (2000b); (32) Ramos-Larios & Phillips (2009); (33) Wareing (2010); (34) Muthu et al. (2000); (35) Rauch (1999); (36) Corradi & Schwarz (1995); (37) Weinberger & Aryal (2004); (38) Aryal et al. (2009); (39) Guerrero et al. (2003); (40) Borkowski (1993); (41) Clark et al. (2010); (42) Chu et al. (1991); (43) Soker & Zucker (1997); (44) Tweedy & Kwitter (1994b); (45) Tweedy & Napiwotzki (1994); (46) Tweedy et al. (1995).References for IPNe distance: (1) Pottasch (1996); (2) Harris et al. (2007); (3) Pottasch & Acker (1998); (4) Acker et al. (1998); (5) Zhang (1993); (6) Sabbadin (1986); (7) Pottasch (1983); (8) Cazetta & Maciel (2001); Kaler & Feibelman (1985); (10) Kaler et al. (1985); (11) Napiwotzki (2001); (12) Napiwotzki (1999); (13) Saurer (1995); (14) Benedict et al. (2009); (15) Rauch et al. (1996); (16) Giammanco et al. (2011); (17) Cahn & Kaler (1971); (18) Ali & Basurah (2008); (19) Napiwotzki & Schonberner (1995); (20) Ali (2006); (21) Bensby & Lundstrom (2001); (22) Mellema (2004); (23) Gathier et al. (1986); (24) Jacoby et al. (1997); (25) Kerber et al. (1998); (26) Hartl & Weinberger (1987); (27) Tajitsu & Tamura (1998); (28) Weinberger & Sabbadin (1981); (29) Werner et al. (1991); (30) Dengel et al. (1980); (31) Cudworth & Peterson (1988); (32) Cudworth (1990); (33) Frew et al. (2010); (34) Rauch et al. (2004).“Ind.” means individual distance, “Ph02” means distances calculated according to Phillips distance scale (2002) and “St.” means statistical distances from literature.References for IPNe radius: (1) ESO-Strasburg Catalog; (2) Ishida & Weinberger (1987); (3) Kerber et al. (2000b); (4) Jacoby & Van de Steene (1995); (5) Jacoby et al. (1997); (6) Kohoutek (1962); (7) Kerber et al. (1998); (8) Kerber et al. (2000a); (9) Melmer & Weinberger (1990); (10) Vauclair et al. (1998); (11) Pierce et al. (2004); (12) Rauch et al. (2004); (13) Tweedy & Kwitter (1996); (14) Borkowski et al. (1990).References for IPNe Expansion Velocity: (1) ESO-Strasburg Catalog; (2) Weinberger (1989); (3) Meaburn et al. (1998); (4) Rodríguez et al. (2001); (5) Pottasch (1996); (6) Guerrero et al. (1998); (7) Phillips (1984); (8) Sabbadin (1984); (9) Hippelein & Weinberger (1990).

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