Impact of electron spectra on morphology of pulsar halos at ultra-high energies-Reference-Cited by-同舟云学术

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Impact of electron spectra on morphology of pulsar halos at ultra-high energies

Published:2024-08 Issue: Volume:43 Page:227-230
ISSN:2214-4048
Container-title:Journal of High Energy Astrophysics
language:en
Short-container-title:Journal of High Energy Astrophysics

Author:

Guo Ying-Ying^ORCID,Yuan Qiang

Publisher

Elsevier BV

Reference28 articles.

1. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth;Abeysekara;Science,2017

2. The Alpha Magnetic Spectrometer (AMS) on the international space station: part II - results from the first seven years;Aguilar;Phys. Rep.,2021

3. Extended very-high-energy gamma-ray emission surrounding PSR J 0622 +3749 observed by LHAASO-KM2A;Aharonian;Phys. Rev. Lett.,2021

4. Very High Energy Cosmic Gamma Radiation: a Crucial Window on the Extreme Universe;Aharonian,2004

5. Detection of spectral hardenings in cosmic-ray boron-to-carbon and boron-to-oxygen flux ratios with DAMPE;Alemanno;Sci. Bull.,2022

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