Notes. Each position reflects a peak of emission in a certain velocity range and one or more tracers and/or a source position: Pos. 1 is the southern HV-blue [O I] peak, closest to the central binary system S106 IR; Pos. 2 is the northern HV-blue [O I] peak; Pos. 3a is the southern cavity blue outflow [O I] peak and the southern HV-red [O I] peak; Pos. 3b corresponds to the YSO S106 FIR, associated with H₂ O maser emission; Pos. 3c is the CO 16 →15 emission peak; Pos. 4 is the northern cavity blue outflow [O I] peak; Pos. 5a is the bulk CO 2 →1 peak located in the dark lane; Pos. 5b is the NW bulk [O I] peak; Pos. 6 is the northern HV-red [O I] peak. The first column for each line gives the intensity in the respective velocity range, the second column the total line integrated (–30 to + 25 km s⁻¹) intensity, and the third column the percentage of how much of the individual velocity integrated line contributes to the total line flux. The last column gives the total FIR flux, determined as explained in Sect. 3.2. The values for the red outflow velocity range (v = 0.5 to 8 km s⁻¹) should be treated with care because the [O I] and [C II] lines suffer from absorption and the CO lines are weak or show no emission. The overall uncertainty of the values given in this table is ~20%. ^(a) In units of (10⁻³ erg s⁻¹ sr⁻¹ cm⁻²). Conversion I(OI) (erg s⁻¹ sr⁻¹ cm⁻²) = 1.0943 10⁻⁴ I(OI) (K km s⁻¹]). ^(b) In units of (10⁻⁵ erg s⁻¹ sr⁻¹ cm⁻²). Conversion I(CII) (erg s⁻¹ sr⁻¹ cm⁻²) = 7.0354 10⁻⁶ I(CII) (K km s⁻¹). Conversion I(CO16-15) (erg s⁻¹ sr⁻¹ cm⁻²) = 6.3953 10⁻⁶ I(CO16-15) (K km s⁻¹). Conversion I(CO11-10) (erg s⁻¹ sr⁻¹ cm⁻²) = 2.0835 10⁻⁶ I(CO11-10) (K km s⁻¹). ^(c) In units of (erg s⁻¹ sr⁻² cm⁻²). ^(d) The total velocity range is from –30 to +25 km s⁻¹.