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Table 9
Intrinsic latitude widths of various Galactic components.
| Component | Width |
|
|
|
| OB stars (Wood & Churchwell 1989)......... |
|
| Dense CS clouds (Bronfman et al. 2000)...... |
|
Free-free via RRLs ( )......... |
|
| Free-free from FastMEM......... |
|
| CO......... |
|
| Dust – FIR (100 μm)......... |
|
| Planck 353, 545, 857 GHz......... |
|
| Gamma-rays (representative of total matter)... |
|
| Synchrotron, GHz frequencies...... |
|
| Synchrotron, K-band polarization...... |
|
| Neutral hydrogen......... |
|
Notes. The widths are the mean values in the longitude range l = 330°–340°, l = 20°–30°, and l = 30°–40°. Values in the 320°–330° range are a factor of ~1.35 ± 0.05 greater.
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