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Table 2

Properties of the observed emission lines on-source (MM1) and at the position of the knots along the jet.

rms V max,b a,* V max,r a,* FWZI b,* V peak c,* T mb,peak d e HVjet/diskf (HVjet/disk)g
(K) (km s-1) (km s-1) (km s-1) (km s-1) (K) (K km s-1) (km s-1) (K km s-1)

CO 3−2
B2 0.3 −16.8 7.3 24.1 33.9 ± 0.3 370.0 ± 1.1 [−8,−15 ] 82.6 ± 0.5
B3 0.3 −16.8 7.7 24.5 73.9 ± 0.3 732.5 ± 0.9 [−8,−15 ] 46.7 ± 0.4
MM1 0.3 −12.9 7.3 20.2 62.9 ± 0.3 424.3 ± 1.0
R2 0.5 −9.5 16.8 26.2 71.1 ± 0.5 567.5 ± 1.6 [ + 10, + 15 ] 43.3 ± 0.7

SiO 8−7
B2 0.5 −16.8 8.6 25.4 −2.6 27.6 ± 0.5 350.2 ± 1.6 [−8,−15 ] 87.0 ± 0.7
B3 0.4 −15.9 11.2 27.1 −4.7 25.2 ± 0.4 294.2 ± 1.3 [−8,−15 ] 30.5 ± 0.6
MM1 0.3 −19.4 15.9 35.3 3.4 11.2 ± 0.3 163.2 ± 1.1
R2 0.4 −7.3 14.2 21.5 9.0 31.8 ± 0.4 252.6 ± 1.1 [ + 10, + 15 ] 32.2 ± 0.5

SO 98−87
B2 0.1 −16.3 6.9 23.2 −8.2 4.4 ± 0.1 49.4 ± 0.4 [−8,−15 ] 18.5 ± 0.2
B3 0.1 −15.1 9.9 24.9 −6.4 13.1 ± 0.1 140.2 ± 0.5 [−8,−15 ] 14.6 ± 0.2
MM1 0.1 −12.9 11.6 24.5 1.1 26.0 ± 0.1 238.1 ± 0.4
R2 0.1 −10.3 12.9 23.2 7.7 11.6 ± 0.1 118.8 ± 0.4 [ + 10, + 15 ] 2.2 ± 0.2

SO282,6−71,7
B2 0.1 −14.1 1.8 15.9 −10.2 0.4 ± 0.1 3.7 ± 0.2 [−8,−10 ] 0.9 ± 0.1
B3 0.1 −11.5 10.9 22.4 −6.5 1.2 ± 0.1 11.6 ± 0.3 [−8,−10 ] 0.8 ± 0.1
MM1 0.1 −6.0 11.3 17.3 1.0 4.4 ± 0.1
R2 0.1 −7.2 10.0 17.2 −1.2 0.6 ± 0.1 5.9 ± 0.2 [ + 8, + 10 ] 0.9 ± 0.1

SO 1011−1010
MM1 0.1 −5.2 4.7 9.9 0.7 ± 0.1 4.2 ± 0.3 [−1.9,−3.5 ] 1.4 ± 0.1
[ + 1.9, + 3.5 ] 0.8 ± 0.1

C17O 3−2
MM1 0.1 −7.7 10.8 18.5 −0.4 7.7 ± 0.1 30.7 ± 0.3 [−1.9,−3.5 ] 5.0 ± 0.1
[ + 1.9, + 3.5 ] 3.2 ± 0.1

Notes.

(*)

Velocities are in terms of VVsys and the error on the velocity values is half of the spectral element i.e. ± 0.2 km s-1.

(a)

Maximum blue- and red-shifted velocity defined as the velocity where the intensity becomes lower than 1 × rms noise.

(b)

Full width at zero intensity FWZI = | Vmax,rVmax,b |.

(c)

Velocity at the emission peak. No value is reported for lines affected by self-absorption, i.e. CO 3−2 and SO 1011−1010.

(d)

Main-beam temperature at the emission peak. For lines affected by self-absorption Tmb,peak could be a lower limit.

(e)

Line intensity integrated over the whole velocity profile (i.e. over the FWZI).

(f)

High-velocity range where jet and disk emission are detected.

(g)

Line intensity integrated over HVjet/disk. For SO 1011−1010 and C17O 3−2, (HVdisk) is measured for both the blue- and the red-shifted line wings.

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