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Table 1:

PNe containing close binary central stars whose nebular morphologies are assessed in this work.
PN G Name Period Diameter Eclipsing i (lit.) Model/i Morphology Traits IRAC Ref.
    (days) (arcsec)   (deg)       1   2  3  4  
005.0+03.0 Pe 1-9 0.14 12 $\times $ 14 Y $\sim$90 - MS L N U N U b
355.3-03.2 PPA 1747-3435 0.22 12 N - - Irr - U U U U a
355.7-03.0 H 1-33 1.13 5 $\times $ 12 N - A/45 CB G U Y U Y a
354.5-03.9 Sab 41 0.30 95 $\times $ 194 N - A/40 LB L, J, R U U U U b
000.6-01.3 Bl 3-15 0.27 4 $\times $ 11 N - A LB G, J Y Y Y Y a
359.1-02.3 M 3-16 0.57 9 $\times $ 13 Y $\sim$90 - Irr L, J Y Y Y Y b
357.6-03.3 H 2-29 0.24 11 $\times $ 14 Y $\sim$90 A/90 CB L, R U U U U b
000.2-01.9 M 2-19 0.67 7 $\times $ 19 N - A/45 CB G, R Y Y Y Y b
358.7-03.0 K 6-34 0.20 14 N - - MS/LB G, L, J?, R N N N Y b
357.0-04.4 PHR 1756-3342 0.26 22 N - B/30 PB - U U U U b
001.8-02.0 PHR 1757-2824 0.80 4 $\times $ 18 Y $\sim$90 A/90 CB - N N N N b
001.2-02.6 PHR 1759-2915 1.10 25 $\times $ 30 Y $\sim$90 A/90 CB - N N N N b
000.5-03.1a MPA 1759-3007 0.50 17 $\times $ 42 N - A/55 LB - U N U N b
001.9-02.5 PPA 1759-2834 0.31 17 $\times $ 35 N - B/45 LB I N N N N b
357.1-05.3 BMP 1800-3408 0.14 30 $\times $ 55 Y $\sim$90 - Irr I U U U U b
000.9-03.3 PHR 1801-2947 0.32 34 N - B/30 PB - N N N N b
001.8-03.7 PHR 1804-2913 6.66 3.5, 8 N - - MS I U N N N b
004.0-02.6 PHR 1804-2645 0.62 24 $\times $ 45 Y $\sim$90 A/90 CB G N N N Y b
144.8+65.8 BE UMa 2.29 180 Y 84 A/85 LB - U U U U j, n
055.4+16.0 A 46 0.47 53 $\times $ 70 Y 80 A/80 LB I U U U U b, c, g
053.8-03.0 A 63 0.46 42 $\times $ 290 Y 88 A/90 CB J U U U U g
136.3+05.5 HFG 1 0.58 540 N 28 - Irr I, L U U U U f
253.5+10.7 K 1-2 0.68 50 $\times $ 130 N $\sim$45 A/45 LB L, J U U U U b, i, m
283.9+09.7 DS 1 0.36 290 $\times $ 335 N 62 - PB I, L U U U U b
329.0+01.9 Sp 1 2.91 120 N - A/5 LB G, R Y Y Y Y c
349.3-01.1 NGC 6337 0.17 60 $\times $100 N 9 A/10 LB G, L, J, R Y Y Y Y l
005.1-08.9 Hf 2-2 0.40 25 N - - MS L, R U U U U b, d
017.3-21.9 A 65 1.00 220 $\times $ 240 N - A/10 LB J U U U U e, h
009.6+10.5 A 41 0.23 15 $\times $ 22 N 66 A/70 CB R U U U U b, g
335.2-03.6 HaTr 4 1.74 24 $\times $ 30 N - B/45 PB - U U U U c
215.6+03.6 NGC 2346 15.99 58 $\times $ 172 N 50 A/50 CB G, R Y Y Y Y c
135.9+55.9 SBS 1150+599A 0.16 4 N - - Irr L? Y Y Y Y k
341.6+13.7 NGC 6026 0.53 60 N 82 - Irr - U U U U d
Morphologies: CB: Canonical bipolar; LB: Likely bipolar; PB: Possible bipolar; MS: Multiple shells; Irr: Irregular.
Morphological Traits: G: Gatley's rule satisfied; I: ISM interaction; L: Low-ionisation knots or filaments; J: Jets; R: Equatorial ring.
IRAC: U: Unavailable; Y: Nebular detection; N: Nebular non-detection.
References: (a) Paper I, (b) this work, (c) Bond & Livio (1990), (d) Schwarz et al. (1992), (e) Walsh & Walton (1996), (f) Heckathorn et al. (1982), (g) Pollacco & Bell (1997), (h) Hua et al. (1998), (i) Corradi et al. (1999), (j) Bond (2000), (k) De Marco (2009), (l) Corradi et al. (2000), (m) Exter et al. (2003), (n) Liebert et al. (1995).

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