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Table 3

Non-detections in AB Aur disk.

Species Frequency rms δv 3σ N(50 K) N(30 K)
(GHz) (mK) (km s-1) (mK cm-2 cm-2
km s-1)

HNC 90.664 4.20 0.65 20.32 2.0 × 1011 1.6 × 1011
DCN* 144.827 9.50 0.40 36.05 7.0 × 1010 6.0 × 1010
217.238 8.00 0.27 24.94 2.3 × 1010 2.5 × 1010
CCH 87.316 6.20 0.67 30.45 1.9 × 1013 1.4 × 1013
DCO+ 144.077 9.20 0.40 34.91 6.0 × 1010 4.6 × 1010
N2H+ 93.171 6.50 0.63 30.96 8.0 × 1012 6.0 × 1012
HC3N 90.979 4.20 0.64 20.16 3.9 × 1011 2.9 × 1011
136.464 7.20 0.43 28.33 1.7 × 1011 2.4 × 1011
c-C3H2 217.822 8.00 0.27 24.94 1.0 × 1011 1.2 × 1011
251.311 7.20 0.23 20.72 8.8 × 1010 1.2 × 1011
p-H2S 216.710 8.60 0.27 26.81 5.4 × 1012 2.7 × 1013
o-H2S 204.140 15.00 0.28 47.62 1.6 × 1016 5.2 × 1016
HCS+ 85.348 5.60 0.69 27.91 1.8 × 1012 1.2 × 1012
256.027 10.00 0.23 28.77 9.7 × 1010 1.1 × 1011
HCO 255.341 10.00 0.23 28.77 1.0 × 1012 1.4 × 1012
265.348 16.00 0.22 45.03 3.2 × 1012 4.5 × 1012
SiO 86.846 6.00 0.67 29.47 4.1 × 1011 3.2 × 1010
217.104 8.50 0.27 26.50 3.5 × 1010 4.9 × 1010
CH3OH 252.485 11.00 0.23 31.65 2.4 × 1013 1.4 × 1014

Notes. The detection limit was calculated assuming a line width of Δv ∼ 4 km s-1. The upper limits on the column densities was calculated with MADEX for a source size of 14 arcsec (2000 AU at 145 pc), a H2 density of 3.5 × 106 cm-3 for two temperatures: 50 and 30 K.

(*)

We used the collisional rates of HCN,

(⋄)

Assuming LTE.

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