Molecular outflows towards O-type young stellar objects

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Table 7:

Total outflow parameters after correction for an inclination angle in the range 30 $^{\circ }{-}60^{\circ }$ ( $\tau _{{\rm m}}$ taken into account).
Source	p	E	$\dot{M}$	$\dot{p}$	$L_{{\rm mec}}$
	( $M_{\odot}$ km s^-1)	(10⁴⁶ erg)	( $10^{-3}~M_{\odot}$ yr^-1)	( $10^{-3}~M_{\odot}$ km s^-1 yr^-1)	( $L_{\odot}$ )
G10.47	4770-8260	40-120	1.4-4.2	12-61	8.3-75
G10.62	1740-3010	15-46	1.4-4.3	13-68	10-92
G16.59	240-410	1.0-3.0	0.32-0.97	1.3-6.8	0.48-4.3
G19.61	7300-12600	73-220	9.8-29	97-500	82-740
G28.87 $^{\rm\dag }$	540-940	4.3-13	0.49-1.5	3.9-20	2.6-24
G35.20	1410-2400	9.2-28	1.1-3.4	7.0-36	3.8-35
G43.89 $^{\rm\dag }$	440-770	3.3-10	1.1-3.3	8.0-42	5.3-48
G48.61	4470-7740	24-71	5.3-16	26-140	12-100
G75.78	1590-2750	12-36	3.0-9.0	22-110	14-130

$^{\rm\dag }$ G28.87 and G43.89 have no $\tau _{{\rm m}}$ estimate.

Source LaTeX | All tables | In the text

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