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Table 5

Outflow properties of B1b-N, B1b-S, GF 9–2, and Cha-MMS1 derived with the vmax method.

Source Lobe (a) (b) tvmax (c) Mobs (d) (e) out (f)
(km s−1) (103 au) (kyr) (10−3 M) (10−6 M km s−1 yr−1) (10−7M yr−1)
B1b-N (1) Red 4.0 0.6 0.7 0.4 0.7 5.7
Blue 4.5 1.3 1.4 1.2 1.2 8.6

B1b-S (1) Red 6.6 3.3 2.4 1.9 2.2 7.9
Blue 7.6 3.0 1.9 3.0 5.4 16

GF 9–2 (2) NE 3.5 2.7 3.6 0.09 0.09 0.3
SW (*) 7.8 6.0 3.6 3.4 8.3 9.4

Cha-MMS1 (**) NE 3.6 2.4 3.1 0.03–0.10 0.04–0.13 0.1–0.3
SW 4.7 2.5 2.5 0.10–0.17 0.2–0.4 0.4–0.7

Notes. (a) Maximum observed velocity ; not corrected for inclination. (b)Projected length of a lobe. (c)Dynamical age . (d) Observed outflow mass. (e)Momentum force . The error only includes the uncertainty on the correction factor from Cabrit & Bertout (1992). (f) Outflow rate out = Mobstvmax. (*) The SW lobe contains three components for which we report the maximum observed length and velocity and the sum of the masses, momentum forces, and outflow rates. (**)The ranges givenfor Mobs, , and out for Cha-MMS1 are based on the two optical depth assumptions for CO (τ12 < < 1 and τ12 = 5).

References. (1) Gerin et al. (2015). (2) Furuya et al. (2019).

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