Larger-sample positional analysis of HI gas shows all SN types deviate from random but are mutually consistent and not linked to densest atomic gas concentrations unlike GRBs.
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Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
Larger-sample positional analysis of HI gas shows all SN types deviate from random but are mutually consistent and not linked to densest atomic gas concentrations unlike GRBs.