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Table 4

H2v = 1−0 S(1) fluxes of the knots for each of the four epochs.

Name f 1 f 2 f 3 f 4 R ap Var
MHO (′′)

2233-N 6.47 6.77 6.30 1.87 y
2233-P 1.41 1.51 1.54 1.40 n

2234-A1+A2 4.75 4.48 4.15 4.25 1.17 y
2234-B1 5.67 5.74 5.32 5.70 1.64 n
2234-C 7.24 7.73 7.39 7.63 2.81 y
2234-D1+D2 21.06 20.08 20.10 20.60 3.28 y
2234-E 6.25 7.33 8.20 8.48 2.34 y
2234-G1 1.03 1.35 1.45 1.22 1.87 n
2234-H1 22.55 23.25 23.94 22.61 2.57 y
2234-H2 6.97 6.89 7.12 6.70 1.87 n
2234-H3 3.89 3.98 4.08 3.96 1.40 n
2234-H4 1.83 1.54 1.81 1.86 1.17 n
2234-H5 2.34 2.29 2.40 2.20 1.40 n
2234-H8 2.54 3.01 3.17 2.73 2.34 y

2235-A1 11.86 12.05 14.56 11.33 2.34 y
2235-A2 2.40 2.40 2.93 3.06 1.40 y
2235-B 48.08 46.13 48.30 44.91 3.74 y
2235-C1 3.67 3.00 3.23 3.06 1.87 y
2235-D 1.57 1.31 1.13 1.66 1.87 y
2235-E 6.24 6.50 7.78 6.64 7.02 y
2235-F1 2.41 2.40 2.34 2.42 1.64 n
2235-I1 0.96 1.05 1.14 1.25 1.17 n
2235-I2 0.96 1.21 1.11 1.29 1.40 n
2235-I3 0.60 0.59 0.50 0.57 1.17 n
2235-K 2.46 2.38 2.61 1.64 n
2235-M1 4.46 4.33 4.02 1.17 n
2235-M2 3.37 3.28 2.93 1.40 n
2235-M4 4.20 4.00 3.90 1.17 n
2235-M5 0.93 0.93 1.01 1.17 n

Notes.This is the line emission measured through an aperture with radius Rap (in arcseconds) centred on each knot. MHO 2234-A1+A2 comprises both knots although A1 is only clearly emerging in ep4. The fluxes f1, f2, f3, and f4 are given in units of 10-15 erg s-1 cm-2. The last column shows whether we find the knot flux to be variable or not.

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