Table 1
Source sample.
| Source | α2000.0 | δ2000.0 | Δline | Type |
|---|---|---|---|---|
| [h:m:s] | [°:′:′′] | [′′] | ||
| IRAS 05399-0121 | 05 42 27.7 | −01 20 00.4 | 11.3 | Class 0/I |
| SMM 1 | 05 42 30.9 | −01 20 45.4 | 6.0 | Prestellar |
| SMM 3 | 05 42 45.3 | −01 16 16.0 | 18.7 | Class 0 |
| IRAS 05405-0117 | 05 43 03.0 | −01 16 31.0 | 11.0 | Class 0 |
| SMM 6 | 05 43 05.0 | −01 18 49.3 | 11.4 | Prestellar |
| SMM 7 | 05 43 22.7 | −01 13 55.0 | 12.7 | Prestellar |
Notes. The coordinates refer to the SABOCA 350 μm peak positions of the sources (Miettinen et al. 2012; Miettinen & Offner 2013a,b). The angular offset, Δline, refers to thedistance from these SABOCA peaks to the target positions observed by Miettinen et al. (2010, 2012). The references to the evolutionary stages of the sources are Miettinen et al. (2009, 2010, 2012), Miettinen & Offner (2013a), and Miettinen (2016).
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.