Table 1
Input data for IXPE simulations of molecular clouds.
| Region (a) | Identification (b) | dlos (c) | Polarization properties (d) | |||
|---|---|---|---|---|---|---|
| Center, radius, dproj | P | ϕ | ||||
| (hh:mm:ss.s, dd:mm:ss.s, ″ pc) | (pc) | (%) | (°) | |||
| 17:46:00.6, −28:56:49.2, | 49 | −14 | MC2 | −17 | 25.8% | 73.8° |
| 17:46:05.5, −28:55:40.8 | 44 | −18 | Bridge B2 | −60 | 15.8% | 77.8° |
| 17:46:12.1, −28:53:20.3 | 49 | −25 | Bridge E | −60 | 12.7% | 67.9° |
| 17:46:21.6, −28:54:52.1 | 90 | −27 | G0.11−0.11 | −17 | 55.8% | 61.6° |
| 17:47:30.60, −28:26:36.6 | 121 | −100 | Sgr B2 | −17 | 65.0% | 88.3° |
| 17:44:30.63, −29:27:22.6 | 100 | 71 | Sgr C1 | −74 | 31.1% | 94.6° |
| 17:44:54.93, −29:28:30.4 | 115 | 66 | Sgr C2 | 58 | 34.9% | 99.1° |
| 17:45:12.19, −29:22:22.0 | 146 | 50 | Sgr C3 | −53 | 32.9% | 106.4° |
Notes. (a) Data of the regions for the spectral analysis and IXPE simulations. Positive and negative projected distances mean east and west of the GC. (b) Cross identification with the target names used in Marin et al. (2015). (c)Distance along the line of sight assumed in Marin et al. (2015). See references therein. Positive and negative means behind and in front of the Galactic plane. (d)Polarization properties from the model of Marin et al. (2015).
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