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Table A.3.

Spectral classification and key lines of CSPNs sample.

N Name S.T. He II 4542 He II 4686 He II 5412 He I 4471 Hβ 4861 N V 4603–19 C IV 5801–12 N.S. Fig.
1 A 33 DAO A A A A y A.19
2 A 50 O(H) III–V A A y A.16
3 A 51 O(H)3–5 Vz A A A A E n A.5
4 A 68 H-rich y A.20
5 AMU 1 O(H)3 Vz A A A A A N/D y A.1
6 Ap 1–12 B0 I–III A A A n A.13
7 BMP J1800-3408 O(H)4–5 Vz A A A A N/D n A.6
8 ESO 216–2 O(H)4–5 V A A A A E y A.5
9 H 1–56 O? A? A? N/D n A.22
10 H 1–65 O(H)8–9 I A E N/D A N/D n A.10
11 H 2–29 O(H) A A A A N/D n A.15
12 H 2–48 O III–V A A A A n A.18
13 HaTr 6 H-rich A n A.20
14 HbDs 1 O(H)3 Vz A A A A E E y A.1
15 He 1–2 O9–B0 I A n A.9
16 He 2–47 O(H)7–9 I A E A ? A n A.10
17 He 2–107 O(H)4 Ifc A E A A A? A+E? y A.4
18 He 2–123 O3–4 A A? N/D n A.18
19 He 2–151 B0 A A A A A? A n A.14
20 He 2–162 B0 I–III A A A A n A.13
21 He 2–182 O(H)4–8 III–V A A A A n A.11
22 IC 2448 O(H)3 III–V A A A A A E y A.4
23 IC 2501 O3-6 A A? A? E n A.8
24 IC 4673 O(H)8 N/D A A N/D y A.10
25 IPHAS 190438 B[e] E n A.14
26 IPHAS 191716 O(H) III–V(e) A A A? A y A.16
27 IPHAS 194751 B0 I A A? n A.12
28 K 3–5 emission line? E? E? E? E? E? n A.24
29 K 3–14 O8–9 A A A n A.9
30 K 3–21 cont. n A.23
31 K 3–36 O? A? E n A.22
32 K 3–66 O A A n A.18
33 K 4–10 O3–4 A A? A E? n A.4
34 K 4–19 B1 I A A n A.13
35 K 4–50 B? A n A.14
36 K 6–34 O(H)4–6 A A A N/D y A.7
37 Lo 8 O(H)3 Vz A A A A A E y A.2
38 Lo 16 O(H)3–4 Vz ((fc)) A A A A A E y A.3
39 LoTr 8 [WR] E n A.24
40 M 1–5 emission line? E? E? n A.24
41 M 1–6 O6-9 I A A? A n A.8
42 M 1–14 O(H)7–9 A A A n A.15
43 M 1–46 O(H)7 I(fc) A E A A A y A.7
44 M 1–72 cont. n A.23
45 M 2–7 O A? A A n A.18
46 M 2–19 O(H)6–8 III–V A A A A N/D n A.5
47 M 2–47 O3-6 A E? A A? E n A.8
48 M 3–16 O(H)4–6 III–V A A A A A N/D n A.7
49 NeVe 3–2 O(H)4 Vz A A N/D A A? N/D y A.6
50 NGC 6326 O(H)5–8 ((fc)) A A A? A E? y A.11
51 Pe 1–9 O(H) A? A A A? A A? N/D y A.17
52 PHR J0745–3535 cont. y A.23
53 PHR J0809–1650 O(H) III–V A A A A y A.11
54 PHR J0834–2819 DAO A A N/D y A.19
55 PHR J1244–6601 H-rich A n A.20
56 PHR J1424–5138 O(H)3 I A N/D A A A E y A.2
57 PHR J1510–6754 O(H)e E E E E E N/D y A.16
58 PHR J1736–3659 O(H)8 If A E N/D A A N/D y A.10
59 PHR J1744–3355 H-rich A N/D y A.20
60 PHR J1756–3342 O(H)3–4 Vz A A A A A N/D y A.3
61 PHR J1757–2824 O(H) A A A N/D y A.17
62 PHR J1804–2913 O(H) A A N/D n A.17
63 PM 1–29 B0.5 I A A n A.12
64 PM 1–295 O(H)9 I A A n A.12
65 PPA J1747–3435 O(H) A A A A N/D n A.15
66 PPA J1855–2328 O(H)6 III–V A A A A n A.7
67 RCW 24 DA A N/D y A.19
68 Sa 1–8 O(H)4–8 III A A A E n A.11
69 Sa 3–96 H-rich? A y A.21
70 Sa 4–1 O(H)3 V A A A A A E y A.1
71 SAB 41 H-rich A y A.21
72 SB 20 O(H)3–4 A N/D A A A E y A.3
73 Sp 1 O(H)3–5 (fc) A A+E? A A E? N/D y A.6
74 Sp 4–1 O? A? E n A.22
75 TS 01 O(H) III–V A A N/D A n A.16
76 VBRC 7 H-rich? N/D A y A.21
77 Vy 2–3 O(H)3–4 I A E? A - A? A E n A.2
78 WKK 136–337 O(H)3 III–V A A N/D - A A N/D y A.3

Notes. The N.S. column indicates whether or not it was possible to subtract the nebular component. The letters A and E indicate whether the ion was in absorption or emission, respectively. An undetected ion was denoted (–), and N/D means no data available in the corresponding spectral range.

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