Multi-waveband photons and high energy neutrinos from the Crab nebula
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/200810871/pdf
Reference45 articles.
1. Does the inverse Compton mechanism alone explain the GeV/TeV gamma-ray emission from the Crab Nebula?
2. The Crab Nebula and Pulsar between 500 GeV and 80 TeV: Observations with the HEGRA Stereoscopic Air Cerenkov Telescopes
3. Observations of the Crab nebula with HESS
4. VHE γ‐Ray Observation of the Crab Nebula and its Pulsar with the MAGIC Telescope
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2. Multiband Emission up to PeV Energy from the Crab Nebula in a Spatially Dependent Lepto-hadronic Model;The Astrophysical Journal;2022-02-01
3. Ultra-high-energy Gamma-Ray Radiation from the Crab Pulsar Wind Nebula;The Astrophysical Journal;2022-01-01
4. PeV Emission of the Crab Nebula: Constraints on the Proton Content in Pulsar Wind and Implications;The Astrophysical Journal;2021-12-01
5. Non-thermal emission and spectral evolution properties of G54.1+0.3;Monthly Notices of the Royal Astronomical Society;2019-06-24
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