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Table 3

LCO PNe dereddeneda fluxes and heliocentric velocities for each lineb.

Object λ obs Ion λ rest Flux/ V helio
(Å) (Å) F(Hβ) (kms-1)

PN2 4339.23 Hγ 4340.47 0.445 –85.9
PN2 4362.1: [O iii] 4363.21 0.178 –75.8:
PN2 4859.96 Hβ 4861.33 1.000 –84.7
PN2 4957.55 [O iii] 4958.91 1.395 –82.4
PN2 5005.47 [O iii] 5006.84 4.142 –82.3
PN2 6560.93 Hα 6562.82 2.812 –86.4
PN2 6581.59 [N ii] 6583.41 0.072 –83.0
PN2 6716.1: [S ii] 6716.47 0.032 19.1:
PN2 6730.8: [S ii] 6730.85 0.021 –1.9:
PN4 4339.47 Hγ 4340.47 0.500 –68.9
PN4 4362.19 [O iii] 4363.21 0.224 –70.1
PN4 4684.70 He ii 4685.68 0.229 –63.4
PN4 4860.25 Hβ 4861.33 1.000 –66.8
PN4 4957.82 [O iii] 4958.91 2.290 –65.8
PN4 5005.74 [O iii] 5006.84 6.651 –66.0
PN4 6561.31 Hα 6562.82 2.809 –69.0
PN4 6581.94 [N ii] 6583.41 0.394 –66.9
PN4 6715.23 [S ii] 6716.47 0.029 –55.3
PN4 6729.41 [S ii] 6730.85 0.059 –64.0
PN4 7134.06 [Ar iii] 7135.78 0.091 –72.4
PN6 4339.37 Hγ 4340.47 0.468 –76.3
PN6 4362.08 [O iii] 4363.21 0.091 –77.8
PN6 4860.09 Hβ 4861.33 1.000 –76.4
PN6 4957.67 [O iii] 4958.91 2.766 –75.1
PN6 5005.61 [O iii] 5006.84 7.257 –73.6
PN6 6561.15 Hα 6562.82 2.804 –76.6
PN6 6581.78 [N ii] 6583.41 0.412 –74.3
PN6 6714.66 [S ii] 6716.47 0.017 –80.9
PN6 6729.05 [S ii] 6730.85 0.235 –80.3
PN6 7133.94 [Ar iii] 7135.78 0.525 –77.0
PN8 4685.29 He ii 4685.68 –1.8
PN8 4860.84 Hβ 4861.33 –7.1
PN8 4958.3: [O iii] 4958.91 –0.2:
PN8 5006.35 [O iii] 5006.84 –6.2
PN8 6562.22 Hα 6562.82 –4.3
PN14 4340.11 Hγ 4340.47 0.062 –25.2
PN14 4362.83 [O iii] 4363.21 0.115 –25.9
PN14 4685.33 He ii 4685.68 0.463 –22.4
PN14 4860.88 Hβ 4861.33 1.000 –27.9
PN14 4958.48 [O iii] 4958.91 3.556 –26.0
PN14 5006.40 [O iii] 5006.84 10.780 –26.1
PN14 6547.49 [N ii] 6548.03 1.347 –24.7
PN14 6562.21 Hα 6562.82 2.797 –27.8
PN14 6582.86 [N ii] 6583.41 3.966 –25.3
PN14 6715.82 [S ii] 6716.47 0.036 –28.9
PN14 6730.25 [S ii] 6730.85 0.039 –26.7
PN14 7135.13 [Ar iii] 7135.78 0.064 –27.5
PN20 4860.40 Hβ 4861.33 –33.8
PN20 4958.03 [O iii] 4958.91 –29.7
PN20 5005.91 [O iii] 5006.84 –32.2

Notes.

(a)

Fluxes dereddened by using Seaton (1979) reddening law.

(b)

A colon in the wavelength indicates a large uncertainty.

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