SN 2024aecx's rapid near-infrared excess is best explained as an infrared echo from pre-existing dust in a face-on disk roughly 5×10^16 cm from the explosion.
Title resolution pending
1 Pith paper cite this work, alongside 38 external citations. Polarity classification is still indexing.
1
Pith paper citing it
38
external citations · OpenAlex
fields
astro-ph.HE 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
An infrared echo from a circumstellar disk in the hydrogen- and helium-poor SN 2024aecx
SN 2024aecx's rapid near-infrared excess is best explained as an infrared echo from pre-existing dust in a face-on disk roughly 5×10^16 cm from the explosion.