H2 distribution during 2-phase Molecular Cloud Formation
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🌌 astro-ph.IM
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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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