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Table B.1

CO line intensities, in K km s−1, used in the modelling.

Star J = 1− 0 J = 2− 1 J = 3−2 J = 4−3 J = 6−5 N
VX Sgr 32.5 (a) 94.5 (a) 99.7 (b) 3
U Her 2.1 (c) 7.3 (d) 8.0 (b), 4.9 (d) 4
RR Aql 2.9 (e) 11.8 (f) 13.7 (f) 11.7 (b) 4
W Hya 12.1 (f) 36.5 (f) 52.7 (b) 3
R Hya 9.7 (f), 17.0 (c) 30.2 (f), 41.5 (a) 44.9 (b) 51.7 (a) 6
RS Vir 2.3 (e) 19.5 (e) 6.2 (b) 3
R Leo 2.4 (g), 4.1 (h) 14.9 (f) 40.0 (f) 50.4 (b) 5
R Aql 19.9 (f) 35.6 (f), 45.0 (d) 47.4 (b), 36.9 (d) 5
R Dor 37.5 (f) 64.1 (f) 98.1 (b) 120 (i) 4
R Crt 5.0 (j) 22.0 (f), 24.0 (j) 26.7 (f), 39.2 (j) 37.0 (b), 54.1 (j) 7
RT Vir 5.2 (j) 11.8 (f), 14.1 (j) 13.5 (f), 19.0 (j) 14.4 (b), 16.1 (j) 7

References. (a)De Beck et al. (2010). (b) J = 4−3 values determined in this work. (c)Josselin et al. (1998). (d)Young (1995). (e) Groenewegen et al. (1999). (f)APEX pointing data: http://www.apex-telescope.org/observing/pointing/spectra. (g) Olofsson et al. (1998). (h) Teyssier et al. (2006). (i) Commissioning data for APEX Band 9 (unpublished).(j)Kerschbaum & Olofsson (1999).

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