The Evolution of Dust Mass in the Ejecta of SN1987A
Eli Dwek, Richard G. Arendt

TL;DR
This paper analyzes IR emission from SN1987A's ejecta over several years, revealing rapid formation of silicate and carbon dust, challenging previous models, and confirming supernovae as major sources of silicate dust in the universe.
Contribution
It presents a new interpretation of dust formation in SN1987A, showing rapid silicate and carbon dust formation without extensive cold accretion, aligning with nucleosynthesis constraints.
Findings
Approximately 0.4 Msun of silicate dust formed early on.
Total dust mass increased to about 0.45 Msun by day 8500.
Silicate dust dominates over carbon in the ejecta.
Abstract
We present a new analysis of the infrared (IR) emission from the ejecta of SN1987A covering days 615, 775, 1144, 8515, and 9090 after the explosion. We show that the observations are consistent with the rapid formation of about 0.4 Msun of dust, consisting of mostly silicates, near day 615, and evolving to about 0.45 Msun of composite dust grains consisting of ~0.4 Msun of silicates and ~ 0.05 Msun of amorphous carbon after day ~8500. The proposed scenario challenges previous claims that dust in SN ejecta is predominantly carbon, and that it grew from an initial mass of ~1e-3 Msun, to over 0.5 Msun by cold accretion. It alleviates several problems with previous interpretations of the data: (1) it reconciles the abundances of silicon, magnesium, and carbon with the upper limits imposed by nucleosynthesis calculations; (2) it eliminates the requirement that most of the dust observed…
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