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Table 1

FF test p-values for a comparison between the emission of the different CO isotopologs in each pair of clouds(a).

No temperatu re correction

Clouds CO(1−0) 13CO(1−0) C18O(1−0) CO(2−1) 13CO(2−1) C18O(2−1)
California(b) – Perseus 4.9 × 10−9 4.8 × 10−6 5.2 × 10−1 - - -
California – Orion A 7.8 × 10−10 2.9 × 10−9 9.4 × 10−2 - - -
Perseus – Orion A 2.8 × 10−2 1.7 × 10−2 2.2 × 10−1 4.7 × 10−3 3.9 × 10−3 8.6 × 10−2

With temperat ure correction

Clouds CO(1−0) 13CO(1−0) C18O(1−0) CO(2−1) 13CO(2−1) C18O(2−1)

California – Perseus 2.5 × 10−6 5.0 × 10−6 5.2 × 10−1 - - -
California – Orion A 8.4 × 10−9 2.0 × 10−5 9.7 × 10−2 - - -
Perseus – Orion A 4.9 × 10−1 2.1 × 10−2 3.1 × 10−1 6.7 × 10−1 4.4 × 10−2 3.0 × 10−1

Notes. (a)Boldface values indicate a probability higher than the 0.05 threshold and are consistent with indistinguishable distributions. (b)No J = 2−1 data available for the California cloud.

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