Table 2: Comparison of calculated with observed line ratios (H$\beta $ = 1) from the whole remnant.
Line Obs.1 Obs.2 M1 M2
[OII] 3727+3729 6.74 (>7) 6.7 8.6
[NeIII] 3869+3968 - 0.21 0.58 0.58
[SII] 4069+4076 2.87 1.37 1.6 1.8
[OIII] 4363 0.37 0.14 .27 .33
HeII 4686 - 0.01 0.06 0.04
[OIII] 4959+5007 4.3 3.3 3.6 4.0
[FeII] 5159 - 0.17 0.3 0.26
[NI] 5199+5200 - 0.04 0.1 0.07
[FeIII] 5270 - 0.04 0.2 0.29
[NII] 5755 0.26 0.11 0.4 0.5
HeI 5876 0.15 0.12 0.18 0.19
[OI] 6300+6364 1.75 1.52 1.2 1.05
[NII] 6583+6548 7.16 7.0 4.8 5.4
[SII] 6717 0.5 0.55 0.6 0.5
[SII] 6730 1.12 1.12 1.1 0.83
[SIII] 9069+9532 0.48 - 1.3 1.4
[CI] 9823+9849 0.20 - 0.3 0.46
w(m1) - - 0 3
w(m3) - - 1.3 5
w(m4) - - 1 0
w(m5) - - 0 3
w(m6) - - 1 3
w(m7) - - 0 1
w(m8) - - 1.3 0
w(m9) - - 0 1
1 Dennefeld (1982); merged 1979 spectrum corrected for reddening by c=1.69.
2 Leibowitz & Danziger (1983): dereddened by c=1.46.

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