The Origins of Calcium-rich Supernovae From Disruptions of CO White Dwarfs by Hybrid He–CO White Dwarfs
Calcium-rich explosions are very faint ( M _B ∼ −15.5), type I supernovae (SNe) showing strong Ca lines, mostly observed in old stellar environments. Several models for such SNe have been explored and debated, but none were able to reproduce consistently the observed properties of Ca-rich SNe, nor t...
সংরক্ষণ করুন:
| প্রধান লেখক: | , , , , , |
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| বিন্যাস: | Artigo |
| ভাষা: | Inglês |
| প্রকাশিত: |
IOP Publishing
2023-01-01
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| মালা: | The Astrophysical Journal |
| বিষয়গুলি: | |
| অনলাইন ব্যবহার করুন: | https://doi.org/10.3847/1538-4357/acaf65 |
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