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Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A · 2008 · DOI 10.1093/mnras/staa2898

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astro-ph.HE 1 astro-ph.SR 1

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Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves

astro-ph.SR · 2026-06-25 · unverdicted · novelty 5.0

Post-processing of 44-year adiabatic 3D simulations of common envelope events yields lightcurves with a 3-5 year hot peak from photosphere expansion, dust formation after 1-3 years causing bolometric decline and 400 K plateau, plus predictions of optical thinning in 100-200 years, matching some obse

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  • Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves astro-ph.SR · 2026-06-25 · unverdicted · none · ref 54

    Post-processing of 44-year adiabatic 3D simulations of common envelope events yields lightcurves with a 3-5 year hot peak from photosphere expansion, dust formation after 1-3 years causing bolometric decline and 400 K plateau, plus predictions of optical thinning in 100-200 years, matching some obse

  • Jittering jets promote dust formation in core-collapse supernovae astro-ph.HE · 2025-09-23 · unverdicted · none · ref 12

    Jittering jets in core-collapse supernovae enhance dust formation and imprint jet-shaped morphologies on the dust in remnants, supporting the jittering jets explosion mechanism.