Fonte: Astroparticle Physics. Unidades: IFSC, EEL, IAG, EACH
Assuntos: RAIOS CÓSMICOS, RAIOS GAMA, ANÁLISE DE DADOS, SUPERNOVAS, TELESCÓPIOS, HÁDRONS, ASTROFÍSICA
ABNT
ACERO, Fabio et al. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants. Astroparticle Physics, v. 150, 2023Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2023.102850. Acesso em: 14 nov. 2024.APA
Acero, F., Catalani, F., Dal Pino, E. M. de G., Souza, V. de, Gonçalves, D. A. F., Silva, R. N. da, et al. (2023). Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants. Astroparticle Physics, 150. doi:10.1016/j.astropartphys.2023.102850NLM
Acero F, Catalani F, Dal Pino EM de G, Souza V de, Gonçalves DAF, Silva RN da, Pereira LAS, Viana A. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants [Internet]. Astroparticle Physics. 2023 ; 150[citado 2024 nov. 14 ] Available from: https://doi.org/10.1016/j.astropartphys.2023.102850Vancouver
Acero F, Catalani F, Dal Pino EM de G, Souza V de, Gonçalves DAF, Silva RN da, Pereira LAS, Viana A. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants [Internet]. Astroparticle Physics. 2023 ; 150[citado 2024 nov. 14 ] Available from: https://doi.org/10.1016/j.astropartphys.2023.102850