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Table 1.
Comparison of the GLOSTAR 5.8 GHz emission features from the dust ridge with literature, specifically Immer et al. (2012a).
| Source | Si, 8.4 GHz(a) | Si, 5 GHz(b) | ΘR(a) | Si, 5.8 GHz | ΘR |
|---|---|---|---|---|---|
| [mJy] | [mJy] | [″] | [mJy] | [″] | |
| A | 180 ± 2 | 154 | 5.1 | 120 ± 10 | 15 |
| B | 9 ± 1 | < 9 | 1.8 | 16 ± 3 | 12 |
| C | 10 ± 1 | < 9 | 1.8 | 15 ± 3 | 15 |
| D | 145 ± 20 | 134 | 14.1 (b) | 436 ± 42 | 30 |
| E | 886 ± 57 | 1417 | 32.0 | 1040 ± 10 | 33 |
Notes. Integrated flux densities as well as their angular radii, ΘR, are shown.
(a)
From Immer et al. (2012a)
(b)
from Becker et al. (1994).
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