Molecular outflows towards O-type young stellar objects

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Table 5:

Total outflow energetics.
Source	$\tau _{{\rm m}}$ $^{\rm\dag }$	M		p		E
		( $M_{\odot}$ )		( $M_{\odot}$ km s^-1)		(10⁴⁶ erg)
		$\tau \ll 1$	$\tau _{{\rm m}}$	$\tau \ll 1$	$\tau _{{\rm m}}$	$\tau \ll 1$	$\tau _{{\rm m}}$
G10.47 $^{\rm\ddag }$	3.6	150	570	1110	4130	8.1	30
G10.62	1.9	90	200	670	1510	5.0	12
G16.59	2.1	24	59	85	210	0.31	0.75
G19.61	3.6	200	740	1740	6320	15	55
G28.87 $^{\rm\ddag }$	-	70	-	470	-	3.3	-
G35.20	1.6	110	230	610	1220	3.5	6.9
G43.89	-	62	-	380	-	2.5	-
G48.61	0.9	590	900	2550	3870	11.8	18
G75.78	0.9	140	220	920	1370	6.0	9.0

$^{\rm\dag }$: Mean $\tau$ of the ¹³CO(2-1) line over the blue and red wings.
$^{\rm\ddag }$: Only the blue lobe parameters, for G10.47, and the red lobe parameters, for G28.87, were determined, due to contamination from nearby unrelated clumps.

Source LaTeX | All tables | In the text

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