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Interstellar hydrocarbons: degradation chemistry in diffuse clouds · 2001 · DOI 10.1093/mnras/stac297

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The evolution of C4H and c-C3H2 in molecular cores

astro-ph.GA · 2026-05-09 · unverdicted · novelty 4.0

C4H/H13CO+ and c-C3H2/H13CO+ abundance ratios decrease with molecular core evolution, indicating consumption of small unsaturated hydrocarbons into complex organic molecules.

Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks

astro-ph.GA · 2026-05-18

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The evolution of C4H and c-C3H2 in molecular cores astro-ph.GA · 2026-05-09 · unverdicted · none · ref 2
C4H/H13CO+ and c-C3H2/H13CO+ abundance ratios decrease with molecular core evolution, indicating consumption of small unsaturated hydrocarbons into complex organic molecules.
Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks astro-ph.GA · 2026-05-18 · unreviewed · ref 238

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