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Table 2:

HOCN observed line parameters.

Transition
$\int T_{\rm MB} {\rm d}v$ $V_{\rm LSR}$ $\Delta v$ $T_{\rm MB}$
  (K km s-1) (km s-1) (km s-1) (K)
Barnard 1-b
404-303 0.048(3) 6.77(3) 0.78(6) 0.058(7)
505-404 0.061(4) 6.75(4) 1.20(8) 0.048(7)
707-606 0.019(2) 6.63(3) 0.62(6) 0.029(5)
L1527 (0, 0)
404-303 0.014(2) 6.11(7) 0.86(14) 0.016(5)
505-404 $\leq$0.008     $\leq$0.010
707-606 $\leq$0.006     $\leq$0.007
L1544
404-303 0.028(3) 7.21(3) 0.54(8) 0.049(7)
505-404 $\leq$0.006     $\leq$0.011
707-606 $\leq$0.003     $\leq$0.007
L183
404-303 0.032(3) 2.48(5) 0.92(10) 0.032(6)
505-404 0.013(2) 2.33(2) 0.39(6) 0.030(5)
707-606 $\leq$0.002     $\leq$0.004
IRAS 16293-2422
404-303 0.015(5) 2.76(12) 0.55(19) 0.026(8)
  0.024(6) 4.66(6) 0.54(16) 0.042
505-404 0.026(8) 2.72(11) 0.79(36) 0.031(10)
  0.038(7) 4.08(8) 0.84(21) 0.043
707-606 0.026(5) 2.72(10) 0.91(22) 0.026(8)
  0.037(6) 4.38(8) 1.11(23) 0.031

Notes. Numbers in parentheses are 1$\sigma$ uncertainties in units of the last digits. For non-detections, the upper limit to the integrated intensity (1$\sigma$) and the observed rms are shown. Adopted rest frequencies (MHz) for the 404-303, 505-404, and 707-606 transitions are 83 900.572, 104 874.679, and 146 820.687, respectively, and their corresponding upper energy levels (K) are 10, 15, and 28 (Brünken et al. 2009a). For IRAS 16293-2422, line parameters were obtained for both velocity components (see text).


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