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Table 3

Physical parameters of the central stars of the PNe observed in the present program (excluding those whose spectra are outshone by an A-type companion).

Name Teff Rs log (L/L) d log  vw vrota | 3⟨Bz⟩ | Ref.
[kK] [R] [kpc] [M/yr] [km s-1] [km s-1] [G] [G] [G] Cols. (2)–(8)

NGC 246 150 0.20 4.20 0.50 6.90 3500 >77 < 900 1500 2.3 × 105 5, 7, 9
NGC 1360 97 0.30 3.64 0.93 10.60 1250 ~10 < 1350 23 1210 2, 3
IC 418 39 1.59 3.72 1.20 7.50 700 >56 < 900 12 62 1, 8
NGC 2392 45 1.34 3.82 1.28 8.10 300 ~10 < 1350 11 83 1
LSS 1362 114 0.18 3.70 1.03 8.70 2400 ~10 < 2400 920 7.2 × 104 2, 3
Hen 2-108 34 2.60 3.92 5.80 6.85 700 ~10 < 2100 85 320 4
Hen 2-113 31 2.50 3.72 1.23 6.10 160 ~10 < 360 23 68 6
Hen 2-131 32 3.50 4.07 3.30 6.88 400 ~10 < 450 26 85 4

Notes. The quantity | 3⟨Bz⟩ | is the upper limit of the surface magnetic field derived from our measurements and and is the minimum magnetic field strength at the stellar surface that would be required to shape the nebula according to Eqs. (4) and (5), respectively.

Reference. (1) Ruiz et al. (2013); (2) Traulsen at al. (2005); (3) Herald & Bianchi (2011); (4) Kudritzki et al. (2006); (5) Koesterke et al. (1998); (6) De Marco & Crowther (1998); (7) Bond & Ciardullo (1999); (8) Prinja et al. (2012); (9) Rauch et al. (2003).

(a)

Assuming vrot = 10 km s-1 where no measurements are available.

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