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Table 6
Comparison of rotating molecular winds.
Source | Dist. [pc] | Age [Myr] | M* [M⊙] | RL [au] | j [au km s−1] | λ(a) – | Reference |
---|---|---|---|---|---|---|---|
HH 211 | 280 | 0.02 | 0.05 | 0.014 | 50 | … | Lee et al. (2009, 2018) |
HH 212 | 400 | 0.04 | 0.25 | 0.05 | 10 | 2–6 | Lee et al. (2017); Tabone et al. (2017) |
IRAS 21078+5211 | 1630 | … | ≈5.6 | ≤6–17 | … | 2.4 | Moscadelli et al. (2022) |
HD 163296 | 101 | ≈5 | 2.2 | … | … | … | Klaassen et al. (2013) |
DG Tau b | 140 | ≈1 | 1.1 | 2û5 | ≈65 | 1.6 | Zapata et al. (2015); de Valon et al. (2020) |
SVS13A | 235 | <1 | 0.9 | 7.5 | 6000 | … | Chen et al. (2016) |
NGC 1333 IRAS4C | 235 | <1 | ≈0.2 | 5–15 | 120–210 | 2–6 | Zhang et al. (2018) |
Orion I | 418 | … | ≈5 | >10 | 500 | … | Hirota et al. (2017) |
TMC 1A | 140 | 0.5 | 0.5 | 25 | 200 | … | Bjerkeli et al. (2016) |
CB 26-YSO 1 | 140 | ≈1 | 0.55 | 20–45 | 140 | 1–2 | This paper; Launhardt et al. (2009) |
Notes. Ordered by launch radius RL. (a)Magnetic lever arm parameter , where RA is the Alfvén radius (Blandford & Payne 1982; Ferreira et al. 2006).
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