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Table 5.

Spatial extents measured from FULLCONCAT dataset.

Source RA (16 47) Dec (−45) Offset Size convolved Size deconvolved


Major axis (″) Minor axis (″) Major axis (″) Minor axis (″)
WR A 8.36412 50 45.5948 0.47 2.49 ± 0.07 1.34 ± 0.04 1.82 ± 0.11 0.89 ± 0.08
WR D 6.29738 51 26.6985 0.65 4.96 LAS
WR B 5.34956 51 5.3995 0.40 3.23 ± 0.03 2.32 ± 0.02 2.77 ± 0.04 2.06 ± 0.03
6.98 LAS
WR G 4.05743 51 23.7000 1.57 3.05 ± 0.19 1.19 ± 0.08 2.53 ± 0.24 0.63 ± 0.18
WR I 0.89863 51 20.6974 0.22 1.86 ± 0.07 1.05 ± 0.04 0.80 ± 0.21
WR L 4.20100 51 7.5000 0.14 1.76 ± 0.05 1.13 ± 0.03 0.55 ± 0.34 0.39 ± 0.17
WR S 2.96652 50 19.7997 0.25 2.25 ± 0.26 1.96 ± 0.22 1.74 ± 0.51 1.42 ± 0.65
WR E 6.06807 52 8.6988 0.54 1.78 ± 0.19 1.10 ± 0.12 0.51 ± 0.53 0.47 ± 0.41
WR F 5.20647 52 25.1996 0.25 1.89 ± 0.10 1.06 ± 0.06 0.81 ± 0.30 0.37 ± 0.28
WR M 3.94256 51 38.1000 0.36 2.18 ± 0.17 1.61 ± 0.12 1.49 ± 0.33 1.10 ± 0.4

W16a 6.69880 50 41.0980 1.37 3.66 ± 0.09 2.41 ± 0.06 3.25 ± 0.10 2.18 ± 0.07
W12a 2.19106 50 59.3991 0.61 2.39 ± 0.03 2.05 ± 0.03 1.80 ± 0.05 1.67 ± 0.06
4.81 LAS
W4a 1.44479 50 37.4982 0.47 2.35 ± 0.02 1.55 ± 0.01 1.62 ± 0.03 1.19 ± 0.02
6.91 LAS
W32 3.71289 50 43.8000 0.50 1.78 ± 0.09 1.04 ± 0.05 0.50 ± 0.4 0.31 ± 0.28
W265 6.29597 49 24.2985 0.72 2.46 ± 0.05 1.92 ± 0.04 1.94 ± 0.09 1.44 ± 0.10
12.59 LAS
W237 3.10953 52 19.1998 0.43 2.60 ± 0.04 1.94 ± 0.03 1.97 ± 0.06 1.64 ± 0.04
15.36 LAS
W75 8.93719 49 58.7933 0.22 2.74 ± 0.15 1.46 ± 0.08 2.16 ± 0.19 1.05 ± 0.13
W20 4.68920 51 24.2999 0.50 2.89 ± 0.03 2.21 ± 0.02 2.35 ± 0.04 1.96 ± 0.03
21.05 LAS
W26 5.40679 50 36.5994 0.18 17.04 LAS

W17 6.18210 50 49.4987 0.76 2.52 ± 0.05 2.04 ± 0.04 2.18 ± 0.13 1.38 ± 0.11
W243 7.50460 52 29.3966 0.25 1.75 ± 0.02 1.00 ± 0.01 0.40 ± 0.11

W9 4.14355 50 31.5000 0.58 2.212 ± 0.001 1.235 ± 0.001 1.405 ± 0.002 0.735 ± 0.001
9.39 LAS
D09-R1 9.08253 51 10.1929 0.07 2.37 ± 0.03 1.88 ± 0.02 1.92 ± 0.05 1.24 ± 0.07
12.85 LAS
D09-R2 6.89972 50 37.1977 0.07 2.13 ± 0.05 1.49 ± 0.04 1.45 ± 0.10 0.86 ± 0.13

W15 6.72735 50 28.7980 1.40 3.95 ± 0.10 1.61 ± 0.04 3.55 ± 0.12 1.27 ± 0.06
W10 3.42580 50 35.3999 1.15 2.55 ± 0.22 1.41 ± 0.12 1.90 ± 0.23 0.98 ± 0.22
W18 5.60787 50 50.3993 1.08 3.86 ± 0.67 1.79 ± 0.31 3.47 ± 0.8 1.49 ± 0.4
W19 4.86139 50 57.8998 1.19 3.75 ± 0.16 2.39 ± 0.10 3.35 ± 0.19 2.15 ± 0.13
W1031 1.96137 50 57.8988 1.55 2.90 ± 0.13 2.53 ± 0.11 2.73 ± 0.15 1.87 ± 0.17
W1056 8.70904 51 2.0939 1.01 2.90 ± 0.28 1.28 ± 0.12 2.36 ± 0.36 0.74 ± 0.29

Notes. Spatial extents are given in terms of convolved and deconvolved sizes. Gaussian fits were applied to the stellar sources using the task JMFIT in the software package AIPS. When Gaussian fits could not be applied, a LAS was found instead.

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