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Table 2

Summary of observational results.

Source Molecule Transition I (peak) σ I dV σ (∫I dV) δV VLSR Comments
[Jy] [Jy] [Jy km s−1 ] [Jy km s−1 ] [km s−1] [km s−1]
HD 213985 12CO J = 2-1 7.7E–02 3.2E–02 1.9E–01 8.8E–02 1.02 –29 Tentative detection
J = 1-0 ≤1.1E–01 3.7E–02 ≤3.0E–01 1.0E–01 1.02
13CO J = 1-0 ≤5.1E–02 1.7E–02 ≤1.5E–01 4.8E–02 1.06
TW Cam 12CO J = 2-1 ≤7.5E–02 2.5E–02 ≤3.4E–01 1.1E–01 1.02 ISM contamination
J = 1-0 ≤1.1E–01 3.7E–02 ≤5.1E–01 1.7E–01 1.02 ISM contamination
13CO J = 1-0 ≤6.6E–02 2.2E–02 ≤3.1E–01 1.0E–01 1.06 ISM contamination
RV Tau 12CO J = 2-1 8.7E–02 2.2E–02 2.5E–01 7.3E–02 1.02 21.5 ISM contamination
J = 1-0 ≤7.2E–02 2.4E–02 ≤2.4E–01 8.0E–02 1.02 ISM contamination
13CO J = 1-0 ≤3.6E–02 1.2E–02 ≤1.2E–01 4.0E–02 1.02 ISM contamination
IRAS 05208 –2035 12CO J = 2-1 ≤8.1E–02 2.7E–02 ≤3.7E–01 1.2E–01 1.02
J = 1-0 ≤1.7E–01 5.7E–02 ≤7.8E–01 2.6E–01 1.02
13CO J = 1-0 ≤6.3E–02 2.1E–02 ≤3.0E–01 1.0E–01 1.06
HD 52961 12CO J = 2-1 1.9E+00 1.3E–01 7.6E+00 2.4E–01 0.25 –7.0
J = 1-0 7.4E–01 5.1E–02 3.5E+00 1.3E–01 0.51 –7.0
13CO J = 2-1 6.6E–01 7.9E–02 2.9E+00 1.8E–01 0.53 –7.0
J = 1-0 2.4E–01 2.4E–02 1.2E+00 8.0E–02 0.53 –7.0
U Mon 12CO J = 2-1 9.5E–02 1.9E–02 6.1E–01 8.2E–02 1.02 10.5
J = 1-0 ≤6.9E–02 2.3E–02 ≤3.0E–01 9.9E–02 1.02
13CO J = 2-1 ≤1.8E–01 6.1E–02 ≤7.9E–01 2.6E–01 1.02
J = 1-0 ≤2.9E–02 9.6E–03 ≤1.2E–01 4.1E–02 1.02
HR 4049 12CO J = 2-1 8.8E–01 1.1E–01 3.7E+00 2.4E–01 0.51 –45.0
J = 1-0 2.8E–01 1.1E–01 7.1E–01 3.2E–01 1.02 –45.0
13CO J = 1-0 1.3E–01 3.8E–02 5.4E–01 1.5E–01 1.06 –45.0
IRAS 11472–0800 12CO J = 2-1 4.6E–02 1.5E–02 2.4E–01 8.3E–02 2.03 30.0 ISM contamination
J = 1-0 ≤7.8E–02 2.6E–02 ≤2.2E–01 7.3E–02 1.02 ISM contamination
13CO J = 1-0 ≤3.6E–02 1.2E–02 ≤1.0E–01 3.4E–02 1.02 ISM contamination
V Vul 12CO J = 2-1 ≤8.7E–02 2.9E–02 ≤4.0E–01 1.3E–01 1.02
J = 1-0 ≤1.1E–01 3.7E–02 ≤5.1E–01 1.7E–01 1.02
13CO J = 1-0 ≤5.4E–02 1.8E–02 ≤2.6E–01 8.5E–02 1.06
AU Peg 12CO J = 2-1 ≤1.8E–01 5.9E–02 ≤8.1E–01 2.7E–01 1.02
J = 1-0 ≤1.6E–01 5.5E–02 ≤7.5E–01 2.5E–01 1.02
13CO J = 1-0 ≤8.1E–02 2.7E–02 ≤3.8E–01 1.3E–01 1.06

Notes. Sources with upper limits lack CO detections. VLSR indicates the centroid of the CO line.

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