Table 4: Observed line fluxes ( $W=\int T_{\rm MB}~ {\rm d}V$ in K km s-1), line widths ($\Delta V$ in km s-1) and opacities for the CN 3 $ 7\over 2$-2 $ 5\over 2$ transitions. The frequencies are given in GHz. Upper limits are at $3\sigma $ in line flux. Numbers in brackets are uncertainties in units of the the last decimal place. The hyperfine line widths were taken to be fixed with an estimated error of $\lesssim $30%.
Source 340.265     340.261     340.247    
  W $\Delta V$ $\tau$ W $\Delta V$ $\tau$ W $\Delta V$ $\tau$
AFGL 2591 1.59(14) 2.6 0.06(1) 1.36(14) 2.7 0.05(1) 19.21(15) 3.3 0.55(1)
W3 IRS 5 1.66(33) 2.6 0.06(1) 1.48(13) 2.5 0.06(1) 20.68(37) 3.8 0.51(1)
IRAS 16293 <0.06 ... ... 0.08(2) 0.8 0.02(1) 2.01(11) 1.3 0.26(2)
N1333-I2 0.10(5) 0.9 0.01(<1) 0.11(5) 0.7 0.02(1) 1.29(5) 1.2 0.10(1)
N1333-I4A <0.09 ... ... <0.09 ... ... 1.01(6) 1.2 ...
L1448-C <0.06 ... ... 0.09(7) 1.1 0.01(<1) 1.28(7) 1.4 0.12(2)
L483 0.24(3) 1.1 0.02(1) 0.15(2) 1.1 0.01(<1) 2.78(3) 1.7 0.15(9)
L723 <0.06 ... ... <0.06 ... ... 1.03(3) 1.7 ...
SMM4 0.23(4) 2.2 0.01(<1) 0.22(4) 2.2 0.01(<1) 2.86(4) 2.8 0.10(2)
V1057 Cyg <0.07 ... ... <0.07 ... ... 0.85(3) 1.4 ...
L1489 <0.07 ... ... <0.07 ... ... 0.72(5) 3.6 ...


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