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Table 2
16 analysed sources, their coordinates, and the known parameters from the Herschel HOPS observations.
| Source | RA | Dec | HOPS name (a,b) | Herschel classification(b) | Lbol (b) | Tbol (b) | Menv (b) | Notes |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (L⊙) | (K) | (M⊙) | ||||
| CSO33-a | 05:35:19.41 | −05:15:38.41 | HOPS-56-B | 0 | 23.3 | 48.1 | 0.8 | |
| CSO33-b | 05:35:19.48 | −05:15:33.08 | HOPS-56-A-A/B/C | 0 | 23.3 | 48.1 | 0.8 | triple system |
| CSO33-c | 05:35:19.81 | −05:15:35.22 | V2358 Ori | 0 | 23.3 | 48.1 | 0.8 | |
| FIR6c-a | 05:35:21.36 | −05:13:17.85 | HOPS-409 | 0 | 8.2 | 28.4 | 1.8 | |
| FIR2 | 05:35:24.30 | −05:08:30.74 | HOPS-68 | I | 5.7 | 100.6 | 1.0 | |
| FIR1a-a | 05:35:24.87 | −05:07:54.63 | HOPS-394-B | 0 | 6.6 | 45.5 | 0.2 | |
| FIR1a-b | 05:35:24.05 | −05:07:52.07 | HOPS-394-A | 0 | 6.6 | 45.5 | 0.2 | |
| MMS9-a | 05:35:25.97 | −05:05:43.34 | HOPS-78-A | 0 | 8.9 | 38.1 | 0.2 | |
| MMS9-b | 05:35:26.15 | −05:05:45.80 | HOPS-78-B | 0 | 8.9 | 38.1 | 0.2 | |
| MMS9-c | 05:35:26.18 | −05:05:47.14 | HOPS-78-C | 0 | 8.9 | 38.1 | 0.2 | |
| MMS9-d | 05:35:25.92 | −05:05:47.70 | HOPS-78-D | 0 | 8.9 | 38.1 | 0.2 | no VLA counterpart |
| MMS5 | 05:35:22.47 | −05:01:14.34 | HOPS-88 | 0 | 15.8 | 42.4 | 0.4 | |
| MMS2-a | 05:35:18.34 | −05:00:32.96 | HOPS-92-A-A/B | Flat(d) | 20.1 | 186.3 | 5.6 | binary(c) |
| MMS2-b | 05:35:18.27 | −05:00:33.95 | HOPS-92-B | Flat | 20.1 | 186.3 | 5.6 | |
| CSO3-b | 05:35:16.17 | −05:00:02.50 | HOPS-94 | I | 6.7 | 123 | 0.1 | no 333 GHz counterpart |
| SIMBA-a | 05:35:29.72 | −04:58:48.60 | HOPS-96 | 0 | 6.2 | 35.6 | 1.9 |
Notes. (a) Fischer et al. (2013). (b) Furlan et al. (2016). (c) Tobin et al. (2020). (d) Protostars characterised by a flat spectral energy distribution (SED) in λFλ from ~2 μm to 24 μm.
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