SN 2024abfl is a subluminous Type IIP event from a low-energy Fe-core collapse of a compact 9–10 M⊙ progenitor with only ~0.003 M⊙ of nickel.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.HE 2years
2026 2verdicts
CONDITIONAL 2representative citing papers
Disabling RTI and boxcar mixing in MESA+STELLA models of a 10 M⊙ progenitor reproduces SN 2024abfl’s flat plateau and steep post-plateau drop using previously proposed mass, radius, and energy.
citing papers explorer
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Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
SN 2024abfl is a subluminous Type IIP event from a low-energy Fe-core collapse of a compact 9–10 M⊙ progenitor with only ~0.003 M⊙ of nickel.
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Exploring the effect of mixing in Low-Luminosity Type IIp Supernovae by modeling SN 2024abfl
Disabling RTI and boxcar mixing in MESA+STELLA models of a 10 M⊙ progenitor reproduces SN 2024abfl’s flat plateau and steep post-plateau drop using previously proposed mass, radius, and energy.