Thermal and Nonthermal Emission from a Peculiar Long-duration GRB 211211A
Long-duration GRB 211211A that lacks a supernova emission even down to very stringent limits at such a low redshift z = 0.076 and is associated with kilonova emission, suggests that its physical origin is from a binary compact star merger. By reanalyzing its data observed with the Gamma-Ray Burst Mo...
Spremljeno u:
| Glavni autori: | , , , , |
|---|---|
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2023-01-01
|
| Serija: | The Astrophysical Journal |
| Teme: | |
| Online pristup: | https://doi.org/10.3847/1538-4357/aca969 |
| Oznake: |
Bez oznaka, Budi prvi tko označuje ovaj zapis!
|
