Cargando…
Revealing a peculiar supernova remnant G106.3+2.7 as a petaelectronvolt proton accelerator with X-ray observations
Supernova remnants (SNRs) have long been considered as one of the most promising sources of Galactic cosmic rays. In the SNR paradigm, petaelectronvolt (PeV) proton acceleration may only be feasible at the early evolution stage, lasting a few hundred years, when the SNR shock speed is high. While ev...
Autores principales: | Ge, Chong, Liu, Ruo-Yu, Niu, Shu, Chen, Yang, Wang, Xiang-Yu |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Elsevier
2021
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8454617/ https://www.ncbi.nlm.nih.gov/pubmed/34557765 http://dx.doi.org/10.1016/j.xinn.2021.100118 |
Ejemplares similares
-
Cosmic-ray Acceleration And X-ray Emission In Supernovae Remnants
por: Ballet, J
Publicado: (2001) -
Emission of Kepler's Supernova Remnant Produced by Accelerated Cosmic Rays
por: Berezhko, E G
Publicado: (2005) -
Proceedings of the International Conference on Supernovae : Supernovae and Supernova Remnants
por: Cosmovici, Cristiano
Publicado: (1974) -
Historical supernovae and their remnants
por: Stephenson, F Richard, et al.
Publicado: (2002) -
On cosmic-ray self-generated turbulence of supernova remnant shocks
por: Marcowith, A
Publicado: (2005)