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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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