<%=journal.getQiKanJianCheng_EN()%>
 
    Home | About Journal | Editorial Board | Instruction | Subscribe | Contact Us |  中文
Modern Physics  2021, Vol. 33 Issue (3): 3-9    DOI:
Current Issue | Next Issue | Archive | Adv Search  |  Next Articles  
 Download: PDF (21012 KB)   HTML (1 KB)   Export: BibTeX | EndNote (RIS)      Supporting Info
Abstract 
Service
E-mail this article
Add to my bookshelf
Add to citation manager
E-mail Alert
RSS
Articles by authors
Key words:   
Cite this article:   
$author.xingMing_EN. [J]. Modern Physics, 2021, 33(3): 3-9.
 
[1] 田珍, 利用 ARGO-YBJ 数据对宇宙线前锋面研究与 LHAASO KM2A阵列伽马质子鉴别能力预研, 中国科学院研究生院, 博士 学位论文, 2018
[2] ASγ collaboration, First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source, PRL, 2019, 123:051101
[3] Baade W, Zwicky F. Cosmic rays from super-novae. Astronomy, 1934, 20:259.
[4] Zhang YR, Liu SM, Yuan Q. Anomalous Distributions of Primary Cosmic Rays as Evidence for Time-dependent Particle Acceleration in Supernova Remnants. ApJ, 2017, 844:L3
[5] Zeng HD, Xin YL, Liu SM. Evolution of High-energy Particle Distribution in Supernova Remnants. ApJ, 2019, 874:50
[6] Yuan Q. et al. A Statistical Model for the Gamma-RAY Variability of the Crab Nebula. Apj, 2011, 730:L15
[7] Ohira Y, Kisaka S, Yamazaki R. Pulsar Wind Nebulae inside Supernova Remnants as Cosmic- Ray PeVatrons. MNRAS, 2018, 478:926
No Similar of article
Modern Physics
Copyright © 2007 Editorial office of Modern Physics
Tel:010-88236284 Fax:010-88236766 E-mail:mp@mail.ihep.ac.cn

Support by Beijing Magtech Co.ltd support@magtech.com.cn