The Origins of Calcium-rich Supernovae From Disruptions of CO White Dwarfs by Hybrid He–CO White Dwarfs
Yossef Zenati(Space Telescope Science Institute), A. Rest(Space Telescope Science Institute), Silvia Toonen(University of Amsterdam), Hagai B. Perets(Technion – Israel Institute of Technology), W. V. Jacobson-Galán(University of California, Berkeley), Luc Dessart(Centre National de la Recherche Scientifique)
Cited by 34
Related Papers
Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf
|The Astrophysical Journal|2022|139
SN 2023ixf in Messier 101: Photo-ionization of Dense, Close-in Circumstellar Material in a Nearby Type II Supernova
|The Astrophysical Journal Letters|2023|111
SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
|The Astrophysical Journal Letters|2023|94
An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud
|Nature Astronomy|2022|90
Formation and evolution of hybrid He–CO white dwarfs and their properties
|Monthly Notices of the Royal Astronomical Society|2018|83