Table 2
Polarization parameters of the sources detected in the Ks- and Lp-band.
| ID | Name | pKs [%] | pLp [%] | θKs [°] | θLp [°] | Class |
|
|
||||||
| 1 | IRS 16NE | 2.7 ± 0.6 | 3.3 ± 0.6 | 35 ± 11 | 12 ± 8 | fg |
| 2 | IRS 16C | 4.3 ± 0.6 | 4.5 ± 0.9 | 25 ± 5 | 22 ± 7 | fg |
| 5 | IRS 1C | 8.2 ± 1.0 | 6.6 ± 1.6 | 8 ± 6 | 20 ± 9 | fg |
| 7 | IRS 1NEE | 7.8 ± 0.8 | 5.7 ± 2.3 | 5 ± 5 | 26 ± 14 | fg |
| 8 | IRS 1SE | 7.6 ± 0.8 | 7.1 ± 1.7 | 11 ± 5 | 24 ± 8 | fg |
| 11 | RS788 | 6.1 ± 0.8 | 4.4 ± 0.9 | 11 ± 5 | 16 ± 8 | fg |
| 12 | IRS 16NW | 3.9 ± 0.8 | 3.8 ± 1.1 | 26 ± 10 | 25 ± 10 | fg |
| 184 | IRS 34 | 7.5 ± 0.5 | 4.3 ± 2.4 | 11 ± 5 | 4 ± 24 | fg |
| 187 | IRS 6E | 4.8 ± 0.8 | 3.8 ± 0.5 | 19 ± 8 | 18 ± 5 | fg |
| 195 | IRS 9 | 2.9 ± 0.9 | 4.2 ± 0.5 | 26 ± 16 | 20 ± 5 | int |
| 196 | IRS 16SW3 | 2.7 ± 0.9 | 3.5 ± 1.6 | 17 ± 17 | –6 ± 23 | int |
| 197 | IRS 16SWE | 3.9 ± 1.0 | 4.1 ± 0.8 | 24 ± 9 | 25 ± 6 | fg |
| 199 | IRS 16SW2 | 2.1 ± 0.9 | 4.9 ± 3.0 | 4 ± 19 | –20 ± 21 | int |
| 201 | IRS 35 | 6.2 ± 0.9 | 5.1 ± 3.1 | 26 ± 5 | 21 ± 22 | fg |
| 284 | IRS 16SW1 | 3.1 ± 0.7 | 6.1 ± 0.7 | 20 ± 14 | 21 ± 5 | int |
| 300 | IRS 29 | 2.8 ± 0.8 | 3.2 ±0.5 | 24 ± 11 | 19 ± 5 | fg |
| 305 | RS1378 | 5.0 ± 0.7 | 3.9 ± 2.8 | 25 ± 5 | 28 ± 25 | fg |
| 389 | RS3909 | 5.6 ± 0.5 | 5.2 ± 0.5 | 30 ± 5 | 18 ± 5 | fg |
| 399 | IRS 5NE | 7.4 ± 0.5 | 8.8 ± 0.9 | 13 ± 5 | 25 ± 5 | int |
| 400 | RS3078 | 5.2 ± 0.5 | 4.0 ± 3.1 | 17 ± 5 | 35 ± 23 | fg |
| 401 | IRS 5 | 5.4 ± 0.5 | 1.8 ± 0.5 | 24 ± 5 | 14 ± 5 | int |
| 403 | IRS 10W | 2.1 ± 0.5 | 0.9 ± 0.5 | 6 ± 5 | –61 ± 5 | int |
| 404 | IRS 10E* | 5.4 ± 0.5 | 4.7 ± 0.5 | 28 ± 5 | 22 ± 5 | fg |
| 405 | IRS 10E2 | 4.7 ± 0.5 | 5.6 ± 1.2 | 28 ± 5 | 22 ± 7 | fg |
| 406 | IRS 10E1 | 5.3 ± 0.5 | 5.3 ± 2.7 | 32 ± 5 | 18 ± 17 | fg |
| 407 | IRS 10E3 | 5.6 ± 0.5 | 6.1 ± 2.7 | 30 ± 5 | –29 ± 16 | int |
| 411 | RS2257 | 6.4 ± 0.9 | 4.8 ± 2.4 | 15 ± 5 | 26 ± 17 | fg |
| 412 | RS2059 | 6.7 ± 0.5 | 6.0 ± 3.5 | 20 ± 5 | 42 ± 16 | fg |
| 413 | RS2214 | 7.5 ± 0.6 | 5.0 ± 3.1 | 12 ± 5 | –14 ± 24 | fg |
| 414 | RS2245 | 6.8 ± 0.5 | 3.8 ± 1.1 | 18 ± 5 | 11 ± 13 | fg |
| 421 | RS2538 | 5.5 ± 0.5 | 3.1 ± 1.3 | 22 ± 5 | 13 ± 19 | fg |
| 422 | RS1707 | 6.5 ± 0.5 | 4.3 ± 1.1 | 18 ± 5 | 24 ± 9 | fg |
| 424 | RS1644 | 5.5 ± 0.6 | 3.9 ± 2.0 | 19 ± 5 | 10 ± 23 | fg |
| 427 | IRS 7 | 2.9 ± 0.5 | 3.6 ± 0.5 | 13 ± 10 | 21 ± 5 | fg |
| 432 | IRS 30W | 5.9 ± 4.9 | 3.6 ± 1.1 | 24 ± 10 | 19 ± 12 | fg |
| 515 | IRS 3 | 5.8 ± 4.8 | 3.7 ± 0.5 | 10 ± 15 | 16 ± 5 | fg |
| 526 | RS628 | 2.3 ± 0.5 | 7.8 ± 3.9 | 16 ± 8 | 70 ± 13 | int |
Notes.ID indicates the number of the source in the list contained in the online material. Name either lists the GCIRS number of the source or the corresponding source number (RSxxxx) in Schödel et al. (2010). Class gives the classification of the source as intrinsically (int) or foreground (fg) polarized.
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