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Table 5
Intrinsic latitude FWHM of thermal dust emission and related data for four longitude ranges.
| Intrinsic width [degrees] | |||||
| Data |
|
Source of data | |||
| l = 20°–30° | l = 30°–40° | l = 320°–330° | l = 330°–340° | ||
|
|
|||||
| 143 GHz...... |
|
|
|
|
Planck |
| 353 GHz...... |
|
|
|
|
Planck |
| 545 GHz...... |
|
|
|
|
Planck |
| 857 GHz...... |
|
|
|
|
Planck |
| 1249 GHz...... |
|
|
|
|
COBE-DIRBE |
| 2141 GHz...... |
|
|
|
|
COBE-DIRBE |
| 100 μm...... |
|
|
|
|
IRAS |
| 60 μm...... |
|
|
|
|
IRAS |
| 25 μm...... |
|
|
|
|
IRAS |
| 12 μm...... |
|
|
|
|
IRAS |
| Gamma-rays... |
|
|
|
|
Fermi |
| CO...... |
|
|
|
|
Planck Collaboration XIII (2014) |
| CS...... |
|
|
|
|
Bronfman et al. (2000) |
| H i...... |
|
|
|
|
Hartmann & Burton (1997), Dickey & Lockman (1990) |
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