Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs
The binary-driven hypernova (BdHN) model explains long gamma-ray bursts (GRBs) associated with supernovae (SNe) Ic through physical episodes that occur in a binary composed of a carbon-oxygen (CO) star and a neutron star (NS) companion in close orbit. The CO core collapse triggers the cataclysmic ev...
Збережено в:
| Автори: | , , , , |
|---|---|
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
MDPI AG
2023-07-01
|
| Серія: | Universe |
| Предмети: | |
| Онлайн доступ: | https://www.mdpi.com/2218-1997/9/7/332 |
| Теги: |
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|