Table 2
Spectral extraction points for line identification and spectral modeling with XCLASS (Sect. 3.4).
| Source | RA | Dec | Ncore | H30α |
|---|---|---|---|---|
| (J2000) | (J2000) | (cm−2) | ||
| G17 | 18:22:26.370 | −13:30:12.06 | 1.0 × 1025 | ✓ |
| G24 A1 | 18:36:12.544 | −07:12:11.14 | 1.3 × 1024 | ✓ |
| G24 A2(N) | 18:36:12.465 | −07:12:09.61 | 9.9 × 1023 | |
| G24 A2(S) | 18:36:12.471 | −07:12:10.09 | 8.2 × 1023 | |
| G345 Main | 16:59:41.628 | −40:03:43.63 | 9.8 × 1025 | ✓ |
| G345 NW spur | 16:59:41.586 | −40:03:43.15 | 2.3 × 1025 |
Notes. These points coincide with the NH2CHO peak used for each source. Ncore was determined as in Sánchez-Monge et al. (2014) using the continuum intensity at the spectral extraction point assuming a Tdust of 100 K, a dust opacity of 1.0 cm2 g−1 (Ossenkopf & Henning 1994), and a gas-to-dust ratio of 100. Check mark (✓) symbols indicate the detection of H30α emission toward the sub-source. For these sources, the continuum was corrected for free–free emission.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.