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Table 3

H2CO and CH3OH rotational transitions in protoplanetary disks.

Object Distance R(CO) i(CO) Transition Frequency Observed intensities Modelled intensities References
(pc) (AU) (deg) (GHz) (mJy km s-1) (mJy km s-1)

H2CO
GM Aur 140 630 49 303–202 218.222 560 130 1, 2
414–313 281.527 570 410 2
LkCa 15 140 905 52 212–111 140.839 844 110 3, 4
820 5
303–202 218.222 696 280 4
660 2
322–221 218.475 <498 30 4
312–211 225.697 498 480 4
414–313 281.527 1120 810 2
515–414 351.768 5264 1100 4
AS 205 125 250 25 303–202 218.222 <160 27 2, 6
414–313 281.527 <300 78 2
AS 209 125 340 38 303–202 218.222 <210 49 2, 6
414–313 281.527 <480 140 2
V4046 Sgr 73 370 33 303–202 218.222 1001 170 2, 7
414–313 281.527 950 500 2
TW Hya 56 215 6 312–211 225.697 <1026 170 4, 8
414–313 281.527 1220 290 9
515–414 351.768 <726 390 4
540 9
AA Tau 140 995 75 303–202 218.222 <520 340 2, 10
414–313 281.527 160 980 2
DM Tau 140 890 35 212–111 140.839 300 110 3, 11
202–101 145.602 110 83 11
313–212 211.211 480 400 11
303–202 218.222 350 270 2
414–313 281.527 290 790 2
GG Tau 140 800 37 212–111 140.839 340 85 11, 12
202–101 145.602 420 67 11
313–212 211.211 790 320 11
IM Lup 190 900 54 303–202 218.222 530 150 2, 13
414–313 281.527 1370 440 2

CH3OH
GM Aur 140 630 49 422–312 E 218.440 <90 15 1, 14
LkCa 15 140 905 52 202–101 A 96.741 <247 <1.00 3, 4
422–312 E 218.440 <498 30 4
<150 14
505–404 A 241.791 <497 71 4
AS 205 125 250 25 422–312 E 218.440 <180 2.9 2, 6, 14
AS 209 125 340 38 422–312 E 218.440 <250 5.3 2, 6, 14
V4046 Sgr 73 370 33 422–312 E 218.440 <380 18 7, 14
TW Hya 56 215 6 707–606 A 338.409 <362 31 8, 14
AA Tau 140 995 75 422–312 E 218.440 <180 36 10, 14
DM Tau 140 890 35 303–202 A 145.103 <240 20 3, 15
422–312 E 218.440 <100 29 14
IM Lup 190 900 54 422–312 E 218.440 <310 16 13, 14

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