From high-mass starless cores to high-mass protostellar objects

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Table 2:

Parameters for the cold (c) and warm (w) components.
	$T_{\rm {c}}$	$M_{\rm {c}}$	$L_{\rm {c}}$	$L_{\rm {w}}$	$L_{\rm {sm}}$	$\frac{L}{L_{\rm {sm}}}$	M₈₅₀
	[K]	[ $M_{\odot}$ ]	[ $L_{\odot}$ ]	[ $L_{\odot}$ ]	[ $L_{\odot}$ ]		[ $M_{\odot}$ ]
18223-12	31	189	13 849	3898	155	115	452
18223-3	18	212	566	36	54	11	413
18223-s2	16	102	157	-	21	8	169
18223-s1	18	142	372	-	36	10	249

Notes. $T_{\rm {c}}$ , $M_{\rm {c}}$ , $L_{\rm {c}}$ and $L_{\rm {w}}$ are fit results. $L_{\rm {sm}}$ is the submm luminosity (longward of 400 $\mu$ m, and M₈₅₀ is the mass in the derived from only the 850 $\mu$ m flux (see main text).

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