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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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
In NGC 4321, HCN/CO, SFR/CO and SFR/HCN increase from upstream to downstream across spiral arms, indicating density-wave-driven sequences in gas density and star-formation efficiency; trends are weaker in M51.
citing papers explorer
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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.
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From gas to stars along the spiral wave: CO, HCN, and star formation variations across the spiral arms in NGC 4321 and M51
In NGC 4321, HCN/CO, SFR/CO and SFR/HCN increase from upstream to downstream across spiral arms, indicating density-wave-driven sequences in gas density and star-formation efficiency; trends are weaker in M51.