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Table 4

Observed and deconvolved source sizes (arcsec).

Source (a) Major axis Minor axis Position angle (degrees) Deconvolved (b) Model (c) 850–870 μm (d)
IRAS 05358 12.0 (0.5) 9.3 (0.4) −46 (6) 4.4 15.0 30.0
IRAS 16272 15.9 (0.7) 11.8 (0.6) −34 (5) 8.8 18.0 50.0
NGC 6334 I(N) 17.2 (0.5) 12.5 (0.4) 38 (3) 11.3 21.6 42.0
W43 MM1 15.8 (1.6) 12.8 (1.2) −89 (15) 15.5 11.8 27.0
DR21(OH) 12.4 (0.4) 11.1 (0.4) −8 (11) 5.4 28.8 33.0
W3 IRS5 14.1 (0.3) 12.0 (0.3) −9 (5) 7.8 40.0 57.0
IRAS 18089 11.0 (0.9) 9.5 (0.8) −37 (21) -0- ... 17.0
W33A 11.6 (0.7) 10.0 (0.6) −44 (16) 5.1 ... 30.0
AFGL 2591 11.3 (0.6) 9.7 (0.5) 76 (12) 3.8 25.2 25.2
G327-0.6 14.3 (0.5) 10.2 (0.4) 67 (4) 5.5 ... 24.0
NGC 6334I 16.1 (0.5) 15.0 (0.4) 88 (13) 12.6 ... 40.0
G29.96 10.7 (0.3) 9.6 (0.3) −13 (11) 3.0 ... 16.0
G31.41 9.9 (0.9) 7.5 (0.7) −5 (13) -0- ... 15.0
G5.89 10.9 (0.2) 10.0 (0.2) −29 (7) 3.9 ... 28.0
G10.47 11.9 (0.7) 10.2 (0.6) −47 (14) 5.5 ... 10.0
G34.26 22.4 (1.0) 16.9 (0.8) −17 (4) 16.9 ... 25.0
W51N-e1 14.5 (0.7) 10.9 (0.5) −63 (6) 8.2 ... 27.0

Notes. (a) The source fitting failed for IRAS 18151 and NGC 7538. (b)Equivalent circular axis; a value of zero means that the source is unresolved. (c) From Chavarría et al. (2010) for W3 IRS5, Herpin (priv. comm.) for AFGL 2591; other sources from Herpin et al. (2016). (d) 3σ radii from Van der Tak et al. (2013).

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