Table A.1
Hub-Filament Systems (HFS) at parsec scales: Literature results ordered by mass.
| HFS | MHFS | LHFS (1) | ṀHFS (2) | ṁHFS (3) | References |
|---|---|---|---|---|---|
| [M⊙] | [pc] | [M⊙ Myr−1] | [M⊙ pc−1 Myr−1] | ||
| targets with ṁ estimates | |||||
| DR21 | 15120 | 4.1 | 4150 | 1100 | Schneider et al. (2011); Hu et al. (2021) |
| SDC335.579-0.272 | 5500 | ~1 | 2500 | ~2500 | Peretto et al. (2013) |
| G6.55-0.1 | 4520 | 7.6 | 1778 | 234 | Sen et al. (2024) |
| G323.46-0.08 | 3072 | 2.4 | 1280 | 506 | Ma et al. (2023) |
| G148.24+00.41 | 2100 | 2.2 | 675 | 306 | Rawat et al. (2024) |
| Mon-R2 | >1700(4) | ~1 | 500 | ~500 | Treviño-Morales et al. (2019) |
| OMC-1 | >1500(4) | 0.8 | 385 | 481 | Hacar et al. (2017a) |
| G310.142+0.758 | 1280 | 0.6 | 2400 | 2166 | Yang et al. (2023) |
| G326.607+00.799 | 1099 | 1.38 | 170 | 123 | He et al. (2023) |
| G22-C1 | 590 | 0.39 | 360 | 923 | Yuan et al. (2018) |
| NGC 1333 | 580 | 0.8 | 100 | ~125 | Hacar et al. (2017b); Walsh et al. (2006) |
| SDC13 | ~400 | ~1 | 15 | 25 | Peretto et al. (2014) |
| G14.225-0.506 South | 377 | 1.15 | 130 | 89 | Busquet et al. (2013); Chen et al. (2019) |
| G14.225-0.506 North | 297 | 1.12 | 100 | 116 | Busquet et al. (2013); Chen et al. (2019) |
| Aquila-Rift | >100 | 0.5 | 30 | 60 | Kirk et al. (2013) |
| surveys without ṁ estimates | |||||
| 12× HFS | 1353-18×104 | 0.9-2.46 | — | — | Tokuda et al. (2023) |
| 39× HFS | 200-4900 | 0.48-1.52 | — | — | Morii et al. (2023) |
| 5× HFS | 135-3739 | 0.27-0.95 | — | — | Anderson et al. (2021) |
Notes. (1) When the HFS radius R is provided we estimate the corresponding length as LHFS = 2R. (2) Most accretion measurements are affected by projection effects and are therefore subject of relatively large uncertainties (see Peretto et al. 2014, , for a discussion). (3) Estimated as ṁHFS = ṀHFS /LHFS. (4) Lower mass limit due to the large contribution of stellar objects.
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