Enhanced CO J = 2-1/J = 1-0 ratio as a marker of supernova remnant-molecular cloud interactions: The CASES of W44 and IC 443

Masumichi Seta, Tetsuo Hasegawa, Tetsuo M. Dame, Seiichi Sakamoto, Tomoharu Oka, Toshihiro Handa, Masahiko Hayashi, Jun Ichi Morino, Kazuo Sorai, Kumiko S. Usuda

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