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Table 8:

Outflow parameters from the CO 3-2 mapping.

Source
i Massa $\Delta V_{\rm max}$b $R_{\rm out}$b $t_{\rm d}$b,c $\dot{M}$a,d $F_{\rm CO}^a$,e $L_{\rm kin}$a,f
    ($M_\odot$) (km s-1) (AU) (yr) ($M_\odot$ ($M_\odot$ yr-1 ($L_\odot$)
            yr-1)  km s-1)  
Red lobe      
Ced 110 IRS 4 15 1.4e-2 4.0 2.4e3 2.8e3 4.2e-6 4.6e-5 7e-5
CrA IRAS 32 45 6.6e-2 6.3 9.3e3 7.1e3 9.3e-6 1.3e-4 5.5e-4
HH 100 60 3.6e-1 14.7 > 6.1e3 >2.0e3 <1.5e-4 <4.9e-3 <7.2e-2
RCrA IRS 7 45 1.1e0 23.0 >1e4 >2.1e3 <4.3e-4 <2.2e-2 <5.0e-1
HH46 35 4.3e-1 9.5 >2.5e4 >1.2e4 <3.2e-5 <4.4e-4 <3.1e-3
IRAS 15398-3359 75 2.9e-2 8.2 2.9e3 4.6e3 6.4e-7 6.4e-6 1.6e-5
Blue lobe      
Ced 110 IRS 4 15 5.8e-3 -4.2 - - - - -
CrA IRAS 32 45 1.7e-2 -5.4 4.6e3 4.0e3 4.3e-6 5e-5 1.8e-4
HH 100 60 4.7e-2 -9.7 4.6e3 2.2e3 2.1e-5 4.4e-4 2.9e-4
RCrA IRS 7 45 1.2e0 -15.8 >5e3 >1.5e3 <7.9e-4 <2.7e-2 <2.9e-1
HH46 35 1.4e-1 -7.4 1.4e4 9.0e3 1.5e-5 1.7e-4 9.3e-4
IRAS 15398-3359 75 9.2e-2 0.7 3.9e3 4.1e4 2.2e-6 3.3e-5 1.2e-4

a Corrected for inclination using the average correction factors of Cabrit & Bertout (1990); b not corrected for inclination; c dynamical time scale: $t_{\rm {d}}=R/V_{\rm {max}}$; d mass outflow rate: $\dot{M}=M/t_{\rm {d}}$; e outflow force : $F_{\rm CO}=MV_{\rm {max}}^2/R$; f kinetic luminosity : $L_{\rm kin}= 0.5~MV^3_{\max}/R$.


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