A low energy core-collapse supernova without a hydrogen envelope
Stefano Valenti (1), Andrea Pastorello (1), Enrico Cappellaro (2),, Stefano Benetti (2), Paolo Mazzali (2,3), Jose Manteca (4), Stefan, Taubenberger (3), Nancy Elias-Rosa (5), Rafael Ferrando (6), Avet Harutyunyan, (2,7), Veli-Pekka Hentunen (8,9), Markku Nissinen (8)

TL;DR
This paper reports the discovery of the faintest hydrogen-poor core-collapse supernova, SN2008ha, suggesting such events are more common than previously thought and may be linked to some long-duration gamma-ray bursts.
Contribution
It provides the first evidence of faint, hydrogen-deficient core-collapse supernovae, challenging previous classifications and linking them to gamma-ray bursts.
Findings
SN2008ha is the faintest hydrogen-poor supernova observed.
Some peculiar thermonuclear supernovae may actually be faint core-collapse events.
Faint, hydrogen-stripped supernovae could be connected to certain gamma-ray bursts.
Abstract
The final fate of massive stars depends on many factors, including mass, rotation rate, magnetic fields and metallicity. Theory suggests that some massive stars (initially greater than 25-30 solar masses) end up as Wolf-Rayet stars which are deficient in hydrogen because of mass loss through strong stellar winds. The most massive of these stars have cores which may form a black hole and theory predicts that the resulting explosion produces ejecta of low kinetic energy, a faint optical display and a small mass fraction of radioactive nickel(1,2,3). An alternative origin for low energy supernovae is the collapse of the oxygen-neon core of a relatively lowmass star (7-9 solar masses) through electron capture(4,5). However no weak, hydrogen deficient, core-collapse supernovae are known. Here we report that such faint, low energy core-collapse supernovae do exist, and show that SN2008ha is…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
