Table 6: Predicted CO line intensities (in K km s^-1) for the detached shell around V644 Sco.
Transition $T_{{\rm kin}} [{\rm K}]$

100 200 400

$J=1\rightarrow0$ 6.5 5.8 5.1

$J=2\rightarrow1$ 22.6 22.8 22.6

$J=3\rightarrow2$ 20.7 22.9 25.5

$J=4\rightarrow3$ 7.8 12.5 13.2

$J=6\rightarrow 5$ 0.58 1.2 2.3

$J=7\rightarrow 6$ 0.15 0.41 1.0

$J=8\rightarrow 7$ 0.04 0.15 0.44

**Table 6:** Predicted CO line intensities (in K km s^-1) for the detached shell around V644 Sco.
Transition	$T_{{\rm kin}} [{\rm K}]$
	100	200	400
$J=1\rightarrow0$	6.5	5.8	5.1
$J=2\rightarrow1$	22.6	22.8	22.6
$J=3\rightarrow2$	20.7	22.9	25.5
$J=4\rightarrow3$	7.8	12.5	13.2
$J=6\rightarrow 5$	0.58	1.2	2.3
$J=7\rightarrow 6$	0.15	0.41	1.0
$J=8\rightarrow 7$	0.04	0.15	0.44

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Radiative transfer
	4 Dust modelling
	5 Molecular line modelling
	6 Discussion
	7 Conclusions
	References