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PHYSICAL CONDITIONS IN MOLECULAR CLOUDS IN THE ARM AND INTERARM REGIONS OF M51

PHYSICAL CONDITIONS IN MOLECULAR CLOUDS IN THE ARM AND INTERARM REGIONS OF M51

We report systematic variations in the emission line ratio of the CO J = 2โ€“1 and J = 1โ€“0 transitions (R2โ€“1/1โ€“0) in the grand-design spiral galaxy M51. The R2โ€“1/1โ€“0 ratio shows clear evidence for the evolution of molecular gas from the upstream interarm regions into the spiral arms and back โ€ฆ