Multiple gas phases in supernova remnant IC 443: mapping shocked H$_2$ with VLT/KMOS
MNRAS 518, 2320-2340 (2023) Supernovae and their remnants provide energetic feedback to the ambient interstellar medium (ISM), which is often distributed in multiple gas phases. Among them, warm molecular hydrogen (H$_2$) often dominates the cooling of the shocked molecular ISM, which has been obser...
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