Table 3
Evolutionary parameters.
| ℓ | Σproto | ΣSFR | ΣSFR_LM | ΣSFR_IR | ϵ ⋆ |
| (deg) |
|
|
|
|
(%) |
|
|
|||||
| 19–33 (all) | 72 | 0.9 ± 0.2 | 0.1 | 1.0 ± 0.2 | 0.7 |
| 340–350 (all) | 723 | 0.8 ± 0.2 | 0.1 | 0.4 ± 0.1 | 0.4 |
|
|
|||||
| 19–33 (bar only) | 111 | 1.2 ± 0.3 | 0.2 | 0.5 ± 0.2 | 0.8 |
| 340–350 (bar only) | 111 | 1.5 ± 0.3 | 0.1 | 1.4 ± 0.4 | 0.5 |
| Distance switch: near ⇒ far | |||||
|
|
|||||
| 19–33 (all) | 72 | 0.9 ± 0.2 | – | – | 0.7 |
| 340–350 (all) | 59 | 0.6 ± 0.1 | – | – | 0.4 |
|
|
|||||
| 19–33 (bar only) | 9 | 1.2 ± 0.3 | – | – | 0.8 |
| 340–350 (bar only) | 14 | 1.2 ± 0.3 | – | – | 0.4 |
| Distance switch: far ⇒ near | |||||
|
|
|||||
| 19–33 (all) | 45 | 0.5 ± 0.1 | – | – | 0.7 |
| 340–350 (all) | 71 | 0.8 ± 0.2 | – | – | 0.4 |
|
|
|||||
| 19–33 (bar only) | 35 | 5.5 ± 1.2 | – | – | 0.7 |
| 340–350 (bar only) | 1 | 0.13 ± 0.03 | – | – | 0.6 |
Notes. Values of density of protostellar clumps (second column), ΣSFR (third column), missing ΣSFR_LM due to completeness limits (fourth column), SFR density calculated through IR luminosity as in Li et al. (2010) and the amount of material converted into stars (sixth column), in and outside the Galactic bar. The three sets of rows separated by the double horizontal line report those values for the distance configuration provided in the original catalog (first set), when switching all the distances assigned as “near” into “far” (second set), and “far” into “near” (third set), as described in Sect. 2.3.
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