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Table 2

Integrated fluxes in Jy km s−1 and radii in au of 12CO, 13CO, and C18O.

12CO
13CO
C18O
Name Flux Rgas, 68% Rgas, 90% Flux Rgas, 68% Rgas, 90% Flux Rgas, 68% Rgas, 90%
(Jy km s−1) (au) (au) (Jy km s−1) (au) (au) (Jy km s−1) (au) (au)
AB Aur 52.35 ± 0.30* 232 ± 12 358 ± 12 37.01 ± 0.18 690 ± 35 1118 ± 35 7.50 ± 0.11 370 ± 35 678 ± 40
AK Sco 2.18 ± 0.05 78 ± 4 114 ± 5 0.68 ± 0.04 66 ± 6 97 ± 18 0.27 ± 0.02 52 ± 5 69 ± 11
BH Cep <0.07 <0.07
BO Cep 1.22 ± 0.08 <387 <525 0.35 ± 0.07 <371 <529
CQ Tau 3.44± 0.04 103 ± 3 146 ± 3 1.12 ± 0.04 84 ± 5 113 ± 6 0.60 ± 0.02 65 ± 4 99 ± 7
HD 9672 3.61 ± 0.08 <285 <460 1.37 ± 0.08 <285 <439 0.12 ± 0.04 <231 <347
HD 31648 19.97 ± 0.08 389 ± 36 597 ± 36 7.03 ± 0.08 313 ± 38 467 ± 38 2.16 ± 0.05 237 ± 38 363 ± 38
HD 34282 9.47 ± 0.09 468 ± 17 673 ± 17 3.46 ± 0.05 340 ± 18 483 ± 18 1.89 ± 0.04 324 ± 18 568 ± 40
HD 36112 7.98 ± 0.14 211 ± 6 305 ± 12 1.87 ± 0.07 121 ± 9 192 ± 18 0.78 ± 0.04 103 ± 6 141 ± 15
HD 58647 <0.03 <0.02 <0.02
HD 97048 27.40 ± 0.14 389 ± 45 596 ± 45 15.93 ± 0.11 433 ± 48 615 ± 48 8.41 ± 0.08 366 ± 48 512 ± 48
HD 100453 2.40 ± 0.03 51 ± 5 78 ± 5 0.91 ± 0.02 38 ± 5 56 ± 5 0.37 ± 0.01 39 ± 5 59 ± 10
HD 100546 63.56 ± 0.12 230 ± 6 322 ± 6 13.13 ± 0.08 187 ± 6 256 ± 6 3.35 ± 0.06 127 ± 9 236 ± 16
HD 104237 2.43 ± 0.06 <43 <64 0.64 ± 0.03 <39 <59 0.37 ± 0.03 <46 <69
HD 135344B 20.07 ± 0.18* 158 ± 10 219 ± 10 8.86 ± 0.08* 119 ± 9 171 ± 9 3.55 ± 0.08* 86 ± 9 125 ± 9
HD 139614 2.82 ± 0.05 <130 <179 1.12 ± 0.04 <108 <151
HD 141569 18.43 ± 0.12* 162 ± 9 220 ± 9 1.27 ± 0.13 150 ± 17 193 ± 54 <0.07
HD 142527 27.14 ± 0.10 542 ± 30 793 ± 30 11.88 ± 0.07 334 ± 31 491 ± 31 3.91 ± 0.04 271 ± 31 368 ± 31
HD 142666 4.05 ± 0.03 136 ± 6 186 ± 6 1.51 ± 0.06 <182 <260 0.64 ± 0.04 <164 <236
HD 163296 51.99 ± 0.09 348 ± 13 496 ± 13 16.98 ± 0.07 287 ± 14 400 ± 14 5.96 ± 0.04 228 ± 14 324 ± 14
HD 169142 18.93 ± 0.05 232 ± 8 347 ± 8 6.37 ± 0.04 156 ± 9 230 ± 9 2.93 ± 0.02 129 ± 9 169 ± 9
HD 176386 <0.11 <0.10 <0.07
HD 200775 <0.09 <0.08
HD 245185 2.37 ± 0.10 <221 <396
HD 290764 6.55 ± 0.13* 271 ± 11 386 ± 14 2.95 ± 0.05* 218 ± 17 328 ± 17 1.51 ± 0.05* 188 ± 18 277 ± 23
HR 5999 <0.08 <0.08 <0.06
KK Oph <0.18 <0.07
MWC 297 <0.03 <0.05 <0.02
SV Cep <0.08 <0.08
TY CrA <0.10 <0.10 <0.07
V718 Sco 1.63 ± 0.09 <106 <151 0.86 ± 0.07 <113 <170
V892 Tau 16.18 ± 1.87 171 ± 30 242 ± 126 3.92 ± 0.20 128 ± 9 191 ± 18 0.86 ± 0.10 90 ± 15 123 ± 43
VV Ser <0.24
XY Per <0.08 <0.08
Z CMa <0.11 <0.06 <0.03

Notes. The fluxes with an asterisk are for the J = 3−2 transition, all others are for the J = 2−1 transition. The upper limits are estimated by using three times the noise in a single channel and multiplying this by the width of the channel and the square root of the number of independent measurements, assuming that the emission is coming from a range of 10 km s−1 in velocity and within a single beam. The error on the flux is estimated by multiplying the noise in an empty channel by the width of the channel and the square root of the number of independent measurements in the Keplerian mask and the area over which the integrated fluxes were computed. All integrated fluxes have an additional 10% calibration error.

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