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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Model atmosphere analysis of 25,642 cool white dwarfs from DESI DR1 shows no mass discrepancy for cool DAs, increasing H/He ratios at low temperatures, and rising He-atmosphere fraction below 10,000 K from convective mixing.
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Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves
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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A Detailed Model Atmosphere Analysis of Cool White Dwarfs in DESI DR1
Model atmosphere analysis of 25,642 cool white dwarfs from DESI DR1 shows no mass discrepancy for cool DAs, increasing H/He ratios at low temperatures, and rising He-atmosphere fraction below 10,000 K from convective mixing.