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Table 4

PNe included in our atlas.

N Name PN G RA (J2000) Dec (J2000) Telescope Images Figure
1 IC 5148−50*,† 002.7−52.4 21 59 31.7 −39 22 36.2 E 10 B.1
2 Hb 4 003.1+02.9 17 41 52.7 −24 42 08.0 E 11 B.1
3 SaWe 3*,† 013.8−02.8 18 26 03.1 −18 12 05.6 E 15 B.1
4 HDW 12 014.8−25.6 19 58 13.2 −26 28 15.4 C 3 B.1
5 DeHt 3 019.4−13.6 19 17 04.6 −18 01 34.2 E 17 B.1
6 A 66 019.8−23.7 19 57 31.8 −21 36 36.8 C 8 B.1
7 A 67 043.5−13.4 19 58 29.3 +03 02 22.6 C 3 B.2
8 NGC 246* 118.8−74.7 00 47 03.8 −11 52 21.6 C 3 B.2
9 PHR0615−0025 209.1−08.2 06 15 20.4 −00 25 49.1 C 3 B.2
10 K 1−11 215.6+11.1 07 36 07.7 +02 42 17.2 C 8 B.2
11 PHR0702−0324 217.2+00.9 07 02 34.2 −03 24 34.9 C 3 B.2
12 PHR0705−0924 222.9−01.1 07 05 51.4 −09 24 11.2 C 4 B.2
13 PHR0700−1143 224.3−03.4 07 00 05.8 −11 43 50.9 C 5 B.3
14 PHR0716−1053 225.4+00.4 07 16 08.0 −10 53 06.0 C 6 B.3
15 PHR0711−1238 226.4−01.3 07 11 43.3 −12 38 03.1 C 6 B.3
16 M 1−16 226.7+05.6 07 37 18.9 −09 38 48.1 E 10 B.3
17 PHR0719−1222 227.1+00.5 07 19 46.7 −12 22 46.9 C 3 B.3
18 PHR0727−1259 228.6+01.9 07 27 49.0 −12 59 30.1 C 3 B.3
19 PHR0727−1707 232.1−00.1 07 27 08.3 −17 07 14.2 C 5 B.4
20 PHR0724−1757 232.6−01.0 07 24 43.4 −17 57 51.1 C 3 B.4
21 SaWe 1 233.0−10.1 06 50 41.0 −22 26 09.3 C 3 B.4
22 HaWe 9 236.0−10.6 06 54 29.0 −25 21 11.6 C 6 B.4
23 PHR0730−2151 236.7−01.6 07 30 46.9 −21 51 43.9 C 3 B.4
24 ESO 427−19 239.6−12.0 06 55 12.1 −29 07 28.4 C 3 B.4
25 NGC 2610† 239.6+13.9 08 33 23.5 −16 08 55.9 E 13 B.5
26 PHR0726−2858 242.5−05.9 07 26 04.8 −28 58 23.5 C 4 B.5
27 PRTM 1 243.8−37.1 05 03 01.7 −39 45 44.0 C 3 B.5
28 PHR0742−3247 247.5−04.7 07 42 23.6 −32 47 44.9 C 3 B.5
29 A 23 249.3−05.4 07 43 18.9 −34 45 13.0 C 3 B.5
30 PHR0834−2819 249.8+07.1 08 34 18.1 −28 19 03.0 C 3 B.5
31 PHR0803−3331 250.4−01.3 08 03 12.5 −33 31 01.9 C 4 B.6
32 PHR0736−3901 252.4−08.7 07 36 25.2 −39 01 31.1 C 3 B.6
33 PHR0820−3516 253.9+00.7 08 20 52.4 −35 16 32.9 C 3 B.6
34 VBRC 1 257.5+00.6 08 30 58.0 −38 19 52.3 C 3 B.6
35 Wray 17−1 258.0−15.7 07 14 48.0 −46 57 24.4 C 3 B.6
36 He 2−11 259.1+00.9 08 37 08.2 −39 26 25.5 C 3 B.6
37 Wray 16−20 260.7−03.3 08 23 40.4 −43 12 44.0 C 3 B.7
38 He 2−15 261.6+03.0 08 53 30.6 −40 03 34.4 C 3 B.7
39 NGC 2818 261.9+08.5 09 16 00.5 −36 37 31.6 E 20 B.7
40 Wray 17−18 262.6−04.6 08 23 53.7 −45 31 09.9 E 10 B.7
41 ESO 209−15 263.3−08.8 08 05 10.9 −48 23 30.1 E 20 B.7
42 He 2−7† 264.1−08.1 08 11 31.9 −48 43 14.5 C 3 B.7
43 ESO 259−10 265.1−04.2 08 34 07.0 −47 16 38.1 C 3 B.8
44 PHR0911−4205 265.4+04.2 09 11 48.5 −42 05 09.9 C 4 B.8
45 PHR0927−4347 268.6+05.0 09 27 28.1 −43 47 53.2 C 6 B.8
46 PHR0905−4753 268.9−00.4 09 05 39.6 −47 53 38.0 C 3 B.8
47 He 2−37 274.6+03.5 09 47 24.3 −48 58 19.1 C 3 B.8
48 PHR0924−5506 276.1−03.3 09 24 15.1 −55 06 24.8 C 6 B.8
49 NGC 2899 277.1−03.8 09 27 03.5 −56 06 18.3 E 20 B.9
50 PHR0958−5039 277.1+03.3 09 58 10.2 −50 39 34.9 C 6 B.9
51 Wray 17−31 277.7−03.5 09 31 27.1 −56 17 41.1 E 20 B.9
52 He 2−32 278.5−04.5 09 30 55.9 −57 36 57.8 C 3 B.9
53 PHR0940−5658 279.1−03.1 09 40 52.5 −56 58 00.1 C 3 B.9
54 PHR1010−5146 279.2+03.5 10 10 04.1 −51 46 48.0 C 6 B.9
55 He 2−36 279.6−03.1 09 43 26.0 −57 16 59.7 E 10 B.10
56 Ste 2−1 280.0+02.9 10 11 57.9 −52 38 15.2 C 3 B.10
57 PHR1019−6059 285.5−03.3 10 19 27.6 −60 59 09.9 C 3 B.10
58 PHR1036−5909 286.3−00.7 10 36 09.2 −59 09 20.2 C 6 B.10
59 He 2−55 286.3+02.8 10 48 43.1 −56 03 23.0 E 14 B.10
60 PHR1046−6109 288.4−01.8 10 46 51.1 −61 09 23.0 C 3 B.10
61 Hf 38 288.4+00.3 10 54 34.9 −59 09 48.7 C 3 B.11
62 PHR1058−5853 288.7+00.8 10 58 02.9 −58 53 34.1 C 3 B.11
63 Hf 39 288.9−00.8 10 53 58.9 −60 26 42.0 E 3 B.11
64 Hf 48† 290.1−00.4 11 03 55.6 −60 36 05.6 E 20 B.11
65 Fg 1 290.5+07.9 11 28 35.9 −52 56 06.4 E 10 B.11
66 NGC 3699† 292.6+01.2 11 27 59.2 −59 57 32.0 C 3 B.11
67 He 2−70† 293.6+01.2 11 35 12.6 −60 16 54.1 C 3 B.12
68 BlDz 1 293.6+10.9 11 53 03.8 −50 50 41.8 E 25 B.12
69 NGC 3918 294.6+04.7 11 50 18.9 −57 10 51.4 E 20 B.12
70 He 2−72† 294.9−00.6 11 41 37.9 −62 28 56.9 C 3 B.12
71 NGC 3195 296.6−20.0 10 09 22.0 −80 51 30.6 E 10 B.12
72 He 2−76 298.2−01.7 12 08 26.0 −64 12 12.1 E 13 B.12
73 PHR1221−5907 299.0+03.5 12 21 00.7 −59 07 32.9 C 4 B.13
74 K 1−23 299.0+18.4 12 30 52.0 −44 14 22.2 E 20 B.13
75 Wray 16−121 302.6−00.9 12 48 31.1 −63 49 56.5 C 3 B.13
76 PHR1250−6346 302.7−00.9 12 50 04.4 −63 46 51.9 E 14 B.13
77 Wray 16−122 304.2+05.9 13 00 41.4 −56 53 28.3 C 6 B.13
78 NGC 5189† 307.2−03.4 13 33 41.9 −65 58 28.9 E 20 B.13
79 He 2−99 309.0−04.2 13 52 31.0 −66 23 28.0 E 19 B.14
80 VBRC 5 309.2+01.3 13 43 59.2 −60 49 40.4 C 3 B.14
81 He 2−103 310.7−02.9 14 05 36.9 −64 40 57.0 E 20 B.14
82 LoTr 7 310.8−05.9 14 15 23.1 −67 31 57.6 E 14 B.14
83 PHR1408−6229 311.7−00.9 14 08 47.3 −62 29 57.8 C 3 B.14
84 He 2−111 315.0−00.3 14 33 18.3 −60 49 44.6 E 14 B.14
85 He 2−119† 317.1−05.7 15 10 39.9 −64 40 19.1 E 20 B.15
86 VBRC 6 317.8+03.3 14 41 35.7 −56 15 06.6 E 25 B.15
87 He 2−114 318.3−02.0 15 04 08.8 −60 53 21.2 E 20 B.15
88 He 2−116 318.3−02.5 15 06 00.8 −61 21 24.4 E 10 B.15
89 ESO 135−04 318.4−03.0 15 08 42.8 −61 44 03.9 E 20 B.15
90 IC 4406† 319.6+15.7 14 22 26.5 −44 09 06.0 E 10 B.15
91 He 2−120 321.8+01.9 15 11 56.1 −55 39 51.1 E 10 B.16
92 Mz 1 322.4−02.6 15 34 16.7 −59 08 59.5 E 10 B.16
93 He 2−163 327.8−07.2 16 29 30.3 −59 09 22.3 E 12 B.16
94 He 2−146 328.9−02.4 16 10 40.9 −54 57 31.9 E 20 B.16
95 Mz 2 329.3−02.8 16 14 32.1 −54 57 04.0 E 20 B.16
96 PHR1557−5128 329.7+01.4 15 57 07.4 −51 28 00.8 E 20 B.16
97 He 2−165 331.5−03.9 16 29 59.6 −54 09 36.7 E 12 B.17
98 He 2−164 332.0−03.3 16 29 53.2 −53 23 04.1 E 14 B.17
99 IC 4642 334.3−09.3 17 11 45.4 −55 24 02.4 E 10 B.17
100 Lo 12 340.8+10.8 16 08 26.3 −37 08 48.3 E 20 B.17
101 NGC 6153 341.8+05.4 16 31 30.9 −40 15 22.5 E 14 B.17
102 H 1−3 342.7+00.7 16 53 31.5 −42 39 18.1 E 10 B.17
103 Pe 1−8 342.9−02.0 17 06 22.8 −44 13 12.1 E 10 B.18
104 He 2−207 342.9−04.9 17 19 32.5 −45 53 10.0 E 18 B.18
105 IC 4637 345.4+00.1 17 05 09.0 −40 52 57.1 E 10 B.18
106 K 1−3† 346.9+12.4 16 23 17.3 −31 44 56.9 E 12 B.18
107 K 2−16† 352.9+11.4 16 44 49.1 −28 04 05.4 E 17 B.18
108 Wray 16−411 353.7−12.8 18 26 41.5 −40 29 51.1 E 14 B.18

Notes. The PNe are denoted by their common name and by their PN G designation. Sixth column lists the telescope used in each observation, EABA and CASLEO, indicated by “E” and “C” respectively. Seventh column lists the number of combined images and eighth column shows the figure number for each nebulae. PNe observed by Hua et al. (1998) and Balick (1987) are marked by “*” and objects labelled with “(†)” have probably Hα contamination or only the continuum emission is detected.

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