Herschel-PACS imaging of protostars in the HH 1–2 outflow complex

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Table 2:

Adopted model parameters.
HOPS	L	$\rho_1$ ^a	$R_{\rm env}$	$\theta_{\rm cav}$	$M_{\rm disk}$	i	$A_{\rm V}$
Source	( $L_{\odot}$ )	(g cm^-3)	(AU)	( $^\circ$ )	( $M_{\odot}$ )	( $^\circ$ )
165	12	$7.5\times10^{-16}$	10³	30	$1\times10^{-4}$	20	35
166	23	$1.5\times10^{-15}$	10⁴	25	$5\times10^{-2}$	40	4
168	84	$3.0\times10^{-13}$	10⁴	40	$5\times10^{-2}$	75	0
203	23	$2.6\times10^{-13}$	10⁴	40	$5\times10^{-2}$	75	0

Notes. ^(a) The envelope density at 1 AU in the limit of no rotation.

Source LaTeX | All tables | In the text

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