Table 4: Equivalent widths, intensities, and intensity ratios of the prominent emission lines in the IRS spectra of WR 102ka and WR 102c.
    WR 102ka WR 102c
  Wavelength $-W_\lambda$ $I_{\rm line}$ $-W_\lambda$ $I_{\rm line}$
  [$\mu $m] [$\mu $m] [10-4 erg s-1 cm-2 sr-1] [$\mu $m] [10-4 erg s-1 cm-2 sr-1]
[S  IV] 10.51 <0.002 <0.0085 0.019 2.94
H2 [J=4-2] S(2) 12.28 0.0062 1.06 0.0021 1.49
I 7-6 12.37 0.0036 0.64 0.0016 1.19
[Ne  II] 12.81 0.073 14.7 0.084 73.2
[Ne  III] 15.55 0.0055 1.02 0.036 38.0
H2 [J=3-1] S(1) 17.04 0.0081 1.32 0.0013 1.40
[S  III] 18.7 0.028 4.04 0.047 54.0
[S  IV]/[S  III]   <0.002 0.054
[Ne  III]/[Ne  II]   0.07 0.52
[Ne  III]/[S  III]   0.25 0.76
H2-S(1)/H2-S(2)   1.25 0.94


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