Red dwarf stars as a new source type of galactic cosmic rays
Author:
Affiliation:
1. P.N. Lebedev Physical Institute, RAS Moscow Russia
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202113931
Reference20 articles.
1. An anomalous positron abundance in cosmic rays with energies 1.5–100 GeV
2. PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra
3. First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV
4. Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
5. Cosmic ray transport in the Galaxy: A review
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1. Search for GeV Gamma-Ray Emission from Possible TeV-bright Red Dwarfs with Fermi-LAT;The Astrophysical Journal;2024-04-01
2. Sources of Primary Cosmic Rays at an Energy of ~100 PeV;Bulletin of the Lebedev Physics Institute;2024-01
3. Quantitative study of the hardening in the Alpha Magnetic Spectrometer nuclei spectra at a few hundred GV;Frontiers in Astronomy and Space Sciences;2022-11-11
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