Table 1
Protostars analyzed in this paper and their observed properties based on Furlan et al. (2016).
| HOPS (1) | PBR(2) | RA (deg) | Dec (deg) | Lbol | Tbol | i | Outflow detection | |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (L⊙) | (K) | (deg) | CO J = 3–2, J = 4–3 | CARMA CO J = 1–0 | ||
| 340 | 86.7554 | +0.4393 | 1.85 | 40.6 | Yes | |||
| 341 | 86.7541 | +0.4395 | 2.07 | 39.4 | Blended | |||
| 354 | 88.6011 | +1.7387 | 6.57 | 34.8 | Nearly edge-on | Yes | ||
| 358 | 86.5301 | −0.2250 | 24.96 | 41.7 | Yes | |||
| 359 | 86.8534 | +0.3500 | 10.00 | 36.7 | No | |||
| 372 | 85.3598 | −2.3056 | 4.80 | 37.3 | Confusion | Extended (3) | ||
| 373 | 093003 | 86.6279 | −0.0431 | 5.32 | 36.9 | ~50 | Yes | Extended |
| 394 | 019003 | 83.8497 | −5.1315 | 6.56 | 45.5 | ~30 | Tentative | Extended |
| 397 | 061012 | 85.7036 | −8.2696 | 1.66 | 46.1 | Intermediate | Confusion | Tentative |
| 223 | 85.7019 | −8.2762 | 19.25 | 247.5 | Intermediate | Yes | Extended | |
| 398 | 082005 | 85.3725 | −2.3547 | 1.01 | 23.0 | No | No | |
| 399 | 082012 | 85.3539 | −2.3024 | 6.34 | 31.1 | ~50 | Yes | Extended |
| 400 | 090003 | 85.6885 | −1.2706 | 2.94 | 35.0 | ~30 | No | Compact |
| 401 | 091015 | 86.5319 | −0.2058 | 0.61 | 26.0 | Tentative (4) | No | |
| 402 | 86.5415 | −0.2047 | 0.55 | 24.2 | No | No | ||
| 403 | 093005 | 86.6156 | −0.0149 | 4.14 | 43.9 | ~30 | No | Compact |
| 404 | 097002 | 87.0323 | +0.5641 | 0.95 | 26.1 | No | No | |
| 405 | 119 019 | 85.2436 | −8.0934 | 1.60 | 35.0 | Edge-on | No | Extended |
| 407 | 302 002 | 86.6177 | +0.3242 | 0.71 | 26.8 | ~80 | No | Extended (5) |
Notes. The inclinations and the CARMA CO J = 1–0 detections are based on Tobin et al. (2016). Most sources listed here are the sources which the maps are centered on, except for HOPS 223, 340, and HOPS 402. Additional sources which are (partially) covered by the maps are shown in Figs. C.1 and C.2. (1) Based on Furlan et al. (2016). (2) Based on Stutz et al. (2013). (3) Tentative blended outflow detection. (4)The red-shifted outflow emission detected toward the HOPS 401 map is probably related to HOPS 316/358. (5) Tentative detection, low S/N.
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