Table B.1
List of the most probable set of models for the YSOs/protostars of our catalogue fitted with the Robitaille (2017) model.
| Source | ndata | Best model set | Score | Disk | Envelope | Cavity | Ambient | Inner radius |
|---|---|---|---|---|---|---|---|---|
| LUPUS I | ||||||||
| HGBS_YSO–J153640.0-342145 | 11 | spubhmi | 18.0 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J153927.9-344616 | 18 | spubhmi | 14.0 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J154011.3-351522 | 8 | sp–h-i | 10.8 | Yes | No | No | No | Variable |
| HGBS_YSO–J154017.6-324649 | 9 | spubhmi | 11.5 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J154051.6-342102 | 12 | spubhmi | 18.0 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J154302.3-340908 | 13 | s-pbsmi | 18.0 | No | Power-law | Yes | Yes | Rsub |
| HGBS_YSO–J154512.8-341729 | 15 | sp–s-i | 18.0 | Yes | No | No | No | Rsub |
| HGBS_YSO–J154529.8-342339 | 18 | spubsmi | 12.0 | Yes | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J154644.6-343034 | 12 | spubsmi | 8.2 | Yes | Ulrich | Yes | Yes | Rsub |
| LUPUS III | ||||||||
| HGBS_YSO–J160500.9-391301 | 5 | sp–s-i | 18.0 | Passive | No | No | No | Rsub |
| HGBS_YSO–J160708.4-391407 | 18 | spu-smi | 8.0 | Passive | Ulrich | No | Yes | Rsub |
| HGBS_YSO–J160709.9-391102 | 18 | spubsmi | 13.5 | Passive | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J160711.5-390347 | 18 | spubhmi | 12.0 | Passive | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160822.4-390445 | 18 | spubhmi | 18.0 | Passive | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160825.7-390600 | 17 | sp–s-i | 10.3 | Passive | No | No | No | Rsub |
| HGBS_YSO–J160829.6-390309 | 15 | s-pbhmi | 18.0 | No | Power-law | Yes | Yes | Variable |
| HGBS_YSO–J160830.7-382826 | 11 | spubhmi | 18.0 | Passive | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160836.1-392300 | 18 | sp–smi | 18.0 | Passive | No | No | Yes | Rsub |
| HGBS_YSO–J160854.5-393743 | 13 | s-pbsmi | 18.0 | No | Power-law | Yes | Yes | Rsub |
| HGBS_YSO–J160901.8-390511 | 15 | spubsmi | 6.0 | Passive | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J160917.9-390453 | 14 | spubhmi | 18.0 | Passive | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160948.5-391116 | 17 | sp–s-i | 18.0 | Passive | No | No | No | Rsub |
| HGBS_YSO–J161051.5-385314 | 18 | spubsmi | 8.4 | Passive | Ulrich | Yes | Yes | Rsub |
| LUPUS IV | ||||||||
| HGBS_YSO–J155641.9-421925 | 11 | spubsmi | 18.0 | Yes | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J155730.4-421032 | 11 | s-u-hmi | 14.4 | No | Ulrich | No | Yes | Variable |
| HGBS_YSO–J155746.6-423549 | 12 | spubsmi | 9.0 | Yes | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J155916.5-415712 | 12 | sp–smi | 9.0 | Yes | No | No | Yes | Rsub |
| HGBS_YSO–J160044.6-415530 | 18 | spubhmi | 18.0 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160115.5-415233 | 18 | spubhmi | 7.2 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160234.6-421129 | 14 | spubhmi | 6.0 | Yes | Ulrich | Yes | Yes | Variable |
| HGBS_YSO–J160329.2-414001 | 13 | spubsmi | 6.0 | Yes | Ulrich | Yes | Yes | Rsub |
| HGBS_YSO–J160403.0-413427 | 7 | sp–h-i | 18.0 | Yes | No | No | No | Variable |
| HGBS_YSO–J160913.7-414430 | 8 | sp–s-i | 18.0 | Yes | No | No | No | Rsub |
| HGBS_YSO–J160956.3-420834 | 6 | sp–s-i | 18.0 | Yes | No | No | No | Rsub |
| HGBS_YSO–J161301.6-415255 | 9 | sp–h-i | 18.0 | Yes | No | No | No | Variable |
Notes. The names of the sets of models are those defined in Robitaille (2017). For each model, the presence of disk, envelope, cavity, and ambient medium is indicated. For the envelope, two possible profiles, spherically symmetric power-law or Ulrich (1976) type, are specified. For all models that contain at least a disk, an envelope, or an ambient medium, the inner radius is set to the same value for all components, and is either set to Rsub (the dust sublimation radius) or is variable in the range Rsub–1000 Rsub.
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.