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Table 6:

Gas production rates for components C, B and G.
Date Component Sky Q(CN) Q(C2) Q(C3) log [Q(C2)/Q(CN)] log [Q(C3)/Q(CN)] log [ ${\rm A f} \rho /Q({\rm CN})$]
March 4 C pp $1.12 \times 10^{24}$ -- $1.64 \times 10^{22}$ -- -1.84 -21.98
March 25 B mc $4.49 \times 10^{23}$ -- -- -- -- -22.16
April 11 B mc $3.92 \times 10^{24a}$ $7.59 \times 10^{23a}$ $4.08 \times 10^{22a}$ -0.71 -1.98 -22.27
April 13 B mc $3.77 \times 10^{24a}$ $2.23 \times 10^{23a}$ $2.36 \times 10^{22a}$ -1.23 -2.22 -22.48
April 26 B pp $2.66 \times 10^{24}$ $2.99 \times 10^{23}$ $8.79 \times 10^{21}$ -0.95 -2.48 -22.75
April 29 G pp $9.68 \times 10^{23}$ -- -- -- -- --
May 2 B pp $2.28 \times 10^{24}$ $4.15 \times 10^{23}$ -- -0.95 -- -22.58
a Production rate derived from spectra not acquired under photometric conditions, but mostly clear sky. Whereas these Qs could be not realistic, the quotients log [Q(C2)/Q(CN)] and log [Q(C3)/Q(CN)] are representative of the relative CN, C2 and C3 production rates.

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