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Table 5

Deconvolved parameters of the continuum sources from a 2D-Gaussian fit obtained from the 12m observations in Band 7.

Source Position Wavelength MAxis mAxis Pos ang Spatial size Int Flux Peak Flux Inc
RA, Dec(J2000) mm [marcsec] [marcsec] [°] UA [mJy] [mJy beam−1] [°]
IRAS 15398-3359 15:43:02.24, –34:09:06.72 0.87 306 ± 43 124 ± 54 139 ± 12 45.9 × 18.6 24 ± 1 19 ± 0.5 66 ± 14
IRAS 16059-3857 16:09:18.09, –39:04:53.30 0.84 431 ± 9 262 ± 7 142 ± 2 64.6 × 39.3 507 ± 8 116 ± 2 53 ± 2
J160155-41523 16:01:15.53, –41:52:35.51 0.85 673 ± 33 274 ± 19 154 ± 2 100.9 × 41.1 92 ± 4 11.8 ± 0.5 66 ± 3
Sz 102 16:08:29.72, –39:03:11.42 0.90 190 ± 12 100 ± 14 13 ± 6 28.5 × 15.0 12 ± 1 6.6 ± 0.1 58 ± 3
Merin 28 16:24:51.77, –39:56:32.95 0.85 680 ± 22 253 ± 8 92 ± 1 102.0 × 37.9 124 ± 4 15.3 ± 0.4 68 ± 1

Notes. To obtain the derived disk inclinations, we measured the angle between the plane of the disk and the plane of the sky, so that a face-on disk has i = 0° and an edge-on disk has i = 90°.

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