APEX-CHAMP+ high-J CO observations of low-mass young stellar objects - II. Distribution and origin of warm molecular gas

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Table 6:

¹³CO model predictions.
Source	$\int T_{\rm {MB}} {\rm d}V$		$T_{\rm {peak}}$
	Mod.	Obs.	Mod.	Obs.
TMR 1	3.6	4.3	1.9	1.9
IRAS 12496-7650	7.2	3.3	3.6	1.6
HH 46	1.9	3.9	1.2	2.9
BHR 71	4.7	1.4	2.7	1.2
Ced 110 IRS 4	2.3	5.2^a	1.2	1.9

^a Possible outflow contribution, see Figs. 5 and 13, estimated to be at 25 $\%$ of total integrated intensity.

Source LaTeX | All tables | In the text

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