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Table 7

Outflow parameters.

Source Mass V max R t d F CO L kin
(M) (km s-1) (104 AU) (103 yr) (10-5M (10-4M (L)
yr-1) yr-1 km s-1)

Red Lobes

NGC 2071 0.39 39.0 4.2 1.1 36.3 145 45.8
L1641 S3 MMS 1 0.022 12.0 0.93 0.77 2.8 3.5 0.34
Vela IRS 17 0.27 10.0 3.5 3.5 7.7 7.9 0.64
Vela IRS 19 0.38 13.0 2.1 1.6 23.8 31.9 3.4
IRAS 20050+27201 0.31 14.0 4.9 3.5 8.9 12.8 1.5
Serpens SMM1 0.006 12.5 1.3 1.1 0.5 0.6 0.06

Blue Lobes

NGC 2071 0.41 36.5 42 1.2 35.3 130 38.4
L1641 S3 MMS 1 0.017 14.5 27 1.9 0.9 1.4 0.16
Vela IRS 17 0.31 10.0 42 4.2 4.6 4.6 0.37
Vela IRS 192 0.05 >3.5 27 <7.7 0.7 >0.23 >0.007
IRAS 20050+27201 0.22 14.0 42 3.0 7.4 10.6 1.2
Serpens SMM1 0.005 16.5 9 0.5 1.5 2.6 0.35

Notes. The dynamical time, td, and outflow force, FCO were corrected for inclination using the factors listed in Table 9 as well as a factor of 1.4 to compensate the method in determining Vmax. See text.

(1)

Average over the detected flows in Bachiller et al. (1995) and B08.

(2)

Strongly limited by detection of Vmax.

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