Table 35
Dust masses derived from LABOCA 870 μm emission.
| Source | Mwarm | Mext | Mvir | Rwarm | Rext | nwarm(H2) | next(H2) |
| (103 M⊙) | (103 M⊙) | (103 M⊙) | (pc) | (pc) | (108 cm-3) | (104 cm-3) | |
|
|
|||||||
| 12326–6245 | 0.42 | 1.6 | 3.0 | 0.03 | 0.6 | 6.7 | 3.6 |
| 16060–5146 | 1.9/5.5 | 4.1/12 | 13/23 | 0.04/0.07 | 0.6/1.1 | 12/6.9 | 6.5/3.7 |
| 16065–5158 | 0.51/3.7 | 2.0/14 | 5.9/17 | 0.03/0.08 | 0.6/2.1 | 8.2/3.1 | 1.7/0.63 |
Notes. The first entry gives the mass of the hot component traced by the SED, the second of the whole dust envelope traced at 870 μm and the third column lists the virial masses derived from C17O(3−2) emission. In the last four columns, the radii for the hot compact component (taken from the XCLASS line modeling) and the extended dust emission as well as the H2 number densities for both components are listed. If two values are listed, they indicate near/far distances used for the calculations.
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.