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Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce

Polin, Abigail et al.
arXiv (All) · Papers
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high-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
Faint Type I supernovae blur the boundaries between spectroscopic classes, obscuring their progenitors and explosion mechanisms. One proposed origin is a double detonation, in which ignition of an accreted helium shell triggers the explosion of a carbon oxygen white dwarf. Surviving helium is a dire
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