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脉冲星风云MSH15-52的非热辐射及其内部粒子传播特性

袁梦环 高华曦 金水灵 卢方武

高师理科学刊2025,Vol.45Issue(7):39-42,4.
高师理科学刊2025,Vol.45Issue(7):39-42,4.DOI:10.3969/j.issn.1007-9831.2025.07.008

脉冲星风云MSH15-52的非热辐射及其内部粒子传播特性

Nonthermal radiation and transport properties of the particles within pulsar wind nebula MSH15-52

袁梦环 1高华曦 1金水灵 1卢方武1

作者信息

  • 1. 玉溪师范学院 数理学院,云南 玉溪 653100
  • 折叠

摘要

Abstract

Pulsar wind nebula MSH15-52 is one of the most important TeV gamma-ray sources in the Galaxy,exhibiting distinct non-thermal multi-wavelength radiation characteristics.Based on the spectral evolution model for exploring particle transport and radiation within the pulsar wind nebula,the nonthermal multiband radiation spectrum of MSH 15-52 was reconstructed,and then the transport properties of particles within the nebula were investigated.The model results indicate that the transport of the particles within MSH15-52 is dominated by convection process at the low energies and by diffusion process at the high energies.

关键词

MSH15-52/非热辐射/传播机制

Key words

MSH15-52/nonthermal radiation/particle transport

分类

数理科学

引用本文复制引用

袁梦环,高华曦,金水灵,卢方武..脉冲星风云MSH15-52的非热辐射及其内部粒子传播特性[J].高师理科学刊,2025,45(7):39-42,4.

基金项目

云南省高等学校大学生创新创业训练计划项目(2023A035) (2023A035)

云南省应用基础研究计划联合面上项目(202201AT070234) (202201AT070234)

高师理科学刊

1007-9831

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