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Table 3
Results of 2D Gaussian fits towards the continuum peak of our Oph sources.
| Source | RA | Dec | Size (a) | PA | F0.87mm | S0.87mm (0.′′4) (b) |
|---|---|---|---|---|---|---|
| [J2000.0] | [J2000.0] | (′′) | (°) | (mJy) | (mJy beam−1) | |
| GSS30-IRS1 | 16 26 21.358 | −24 23 04.85 | 0.19 ± 0.02 × 0.12 ± 0.01 | 96 ± 9 | 35.3 ± 0.7 | 30.0 ± 0.3 |
| [GY92] 30 | 16 26 25.475 | −24 23 01.81 | 0.25 ± 0.01 × 0.12 ± 0.01 | 28 ± 1 | 105.0 ± 0.5 | 80.2 ± 0.2 |
| WL 12 | 16 26 44.203 | −24 34 48.86 | 0.14 ± 0.01 × 0.11 ± 0.01 | 60 ± 11 | 160.4 ± 1.0 | 142.4 ± 0.5 |
| LFAM 23 (c) | 16 26 59.166 | −24 34 59.07 | 0.09 ± 0.02 × 0.05 ± 0.04 | 38 ± 45 | 17.6 ± 0.3 | 16.9 ± 0.2 |
| [GY92] 197 | 16 27 05.252 | −24 36 30.14 | 0.44 ± 0.01 × 0.13 ± 0.01 | 169 ± 1 | 128.3 ± 0.6 | 71.1 ± 0.2 |
| Elias 29 | 16 27 09.416 | −24 37 19.20 | 0.17 ± 0.02 × 0.16 ± 0.02 | 61 ± 90 | 41.2 ± 0.6 | 34.1 ± 0.3 |
| IRS 43 VLA 1 | 16 27 26.908 | −24 40 50.67 | 0.21 ± 0.03 × 0.13 ± 0.02 | 96 ± 17 | 41.6 ± 1.9 | 32.1 ± 0.9 |
| IRS 43 VLA 2 | 16 27 26.917 | −24 40 51.18 | 0.36 ± 0.09 × 0.2 ± 0.1 | 150 ± 37 | 7.5 ± 1.0 | 3.7 ± 0.4 |
| IRS 44 | 16 27 27.988 | −24 39 33.93 | 0.24 ± 0.03 × 0.18 ± 0.03 | 124 ± 19 | 38.6 ± 1.2 | 29.1 ± 0.6 |
| IRAS 16253-2429 | 16 28 21.620 | −24 36 24.17 | 0.23 ± 0.02 × 0.13 ± 0.02 | 111 ± 6 | 39.8 ± 0.7 | 31.9 ± 0.4 |
| ISO-Oph 203 | 16 31 52.445 | −24 55 36.48 | 0.14 ± 0.03 × 0.05 ± 0.03 | 107 ± 18 | 11.3 ± 0.3 | 10.6 ± 0.2 |
| IRS 67 A | 16 32 00.989 | −24 56 42.78 | 0.5 ± 0.1 × 0.3 ± 0.2 | 46 ± 17 | 35.7 ± 7.0 | 16.2 ± 2.3 |
| IRS 67 B | 16 32 00.978 | −24 56 43.44 | 0.22 ± 0.02 × 0.14 ± 0.01 | 88 ± 9 | 155.5 ± 4.0 | 125.1 ± 2.0 |
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