**Table 4:** Properties of intermediate-mass outflows.
	M	P	E	$\dot P$
Outflow	( $M_{\odot}$ )	( $M_{\odot}$ km s^-1)	(10⁴⁵ erg)	( $M_\odot ~ \mbox{km s}^{-1}$ yr^-1)
IRAS 20050+2720^a	1.7	25.4	7.7	${\sim} 5.0\times10^{-3}\phantom{13}$
IRAS 21391+5802^b	0.14	3.6	1.2	$1.4\times10^{-3}$
HH288^c	11	385	6.7	$1.4\times10^{-2}$
L1641S^d	1.4	37	0.3	$5.3\times10^{-4}$
NGC 2071^e	10	81	8.5	$5.1\times10^{-3}$

^a The parameters correspond to the whole emission of the different outflow lobes detected in IRAS 20050+2720 (Bachiller et al. 1995). ^b Beltrán et al. (2002). ^c Because of the difficulty of treating each outflow separately, the parameters correspond to the whole emission, thus including the two outflows detected in HH228 (Gueth et al. 2001). ^d Anglada (1995) and Wu et al. (2004). ^e Snell et al. (1984).

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