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Table 1

List of HerPlaNS target PNe.

D R Dyn. age T X-ray
Name PN G Morpha (kpc) (pc) (103 yr) (103 K) Sp. type H2 results

NGC 40 120.0+09.8 Bbsh 1.0 0.11 4 48 [WC8] Y D
NGC 2392 197.8+17.3 Rsai 1.3 0.14 3 47 Of(H) N D, P
NGC 3242 261.0+32.0 Ecspaih 1.0 0.10 4 89 O(H) N D
NGC 6445 008.0+03.9 Mpi 1.4 0.14 3 170 ... Y P
NGC 6543 096.4+29.9 Mcspa 1.5 0.09 5 48 Of-WR(H) N D, P
NGC 6720 063.1+13.9 Ecsh 0.7 0.13 6 148 hgO(H) Y N
NGC 6781 041.802.9 Bth 1.0 0.32 38 110 DAO Y N
NGC 6826 083.5+12.7 Ecsah 1.3 0.08 5 50 O3f(H) N D, P
NGC 7009 037.734.5 Lbspa 1.5 0.09 3 87 O(H) N D, P
NGC 7026b 089.0+00.3 Bs 1.7 0.16 <1 80 [WC] Y D
Mz 3c 331.701.0 Bps 13 0.10.2 0.62 32: ... N D, P

Notes. Adopted from ChanPlaNS Table 1 (Kastner et al. 2012, and references therein), for which data are compiled from Frew (2008). with additional information on H2 (Hora et al. 1999; Smith 2003). X-ray results key: P = point source; D = diffuse source; N = not detected.

(a)

According to the classification scheme by Sahai et al. (2011); B: bipolar, E: elongated, L: collimated lobe pair, M: multipolar, R: round, a: ansae, b: bright (barrel-shaped) central region, c: closed outer lobes, h: halo; i: inner bubble, p: point symmetry, s: CSPN apparent, t: bright central toroidal structure;

(b)

Not a ChanPlaNS target PN; NGC 7026 from Gruendl et al. (2006), and Mz 3 from Kastner et al. (2003). The point spread function of XMM-Newton does not allow us to determine whether or not a point source is present.

(c)

Not a ChanPlaNS target PN; may be a symbiotic/PN mimic (Frew 2008); data from Kastner et al. (2003).

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