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H2 distribution during 2-phase Molecular Cloud Formation

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arxiv 1512.03979 v1 pith:6KW2KFK6 submitted 2015-12-12 astro-ph.IM

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keywords moleculararisecloudcloudscomparedconsequencedistributionduring
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We performed high-resolution, 3D MHD simulations and we compared to observations of translucent molecular clouds. We show that the observed populations of rotational levels of H2 can arise as a consequence of the multi-phase structure of the ISM.

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