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Table 6

Molecular line strengths of H2O, hydroxyl, and CH+ for the sources with at least one detection in these lines.

Star o-H2O o-H2O CH+ o-H2O OH OH CH+/p-H2O CH+/o-H2O o-H2O
λ (μm) 63.32 71.946 72.14 78.74 79.11 79.18 90.00 179.52 180.42
Eup (K) 1071.0 843.5 432.2 296.8 114.4 194.1

AB Aur  < 29.8  < 19.0  < 36.7  < 26.5 24.6: (7.9)  < 24.8  < 18.4  < 13.5  < 8.2
HD 31648 9.8: (2.2)  < 12.4  < 21.6  < 17.7  < 9.9  < 10.3  < 9.1  < 7.5  < 5.9
HD 97048  < 16.4  < 16.8  < 18.6  < 18.2  < 17.0  < 18.9 17.4 (4.9)  < 18.3  < 13.8
HD 100546  < 25.9  < 50.9 127.5 (17.0)  < 57.0  < 41.9  < 42.1 116.0 (16.1) 30.5 (4.8)  < 17.1
HD 163296 14.2: (4.4) 16.5 (5.3)  < 19.9 10.2: (4.1) 11.4 (3.4)  < 9.1 4.7: (1.9)  < 10.4  < 6.2

Notes. Line flux in units of 10-18 W/m2, 1σ continuum rms between brackets in the case of a detection, or, in the case of a non-detection, 3σ upper limits. With “:”, we indicate that the feature is between 2σ and 3σ. At 90 μm and 179.5 μm, there is a possible blend of CH+ and H2O. For the water lines, we also give the upper energy level in K.

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