How unique are pulsar wind nebulae models? Implementation of a multi-parameter, automatic fitting for time-dependent spectra
Author:
Publisher
Elsevier BV
Subject
Astronomy and Astrophysics,Space and Planetary Science
Reference70 articles.
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1. Likely Detection of GeV γ-Ray Emission from Pulsar Wind Nebula G32.64+0.53 with Fermi-LAT;The Astrophysical Journal;2024-08-27
2. Could the TeV emission of starburst galaxies originate from pulsar wind nebulae?;Monthly Notices of the Royal Astronomical Society;2023-11-27
3. Reverberation of pulsar wind nebulae – III. Modelling of the plasma interface empowering a long term radiative evolution;Monthly Notices of the Royal Astronomical Society;2023-08-04
4. Reverberation of pulsar wind nebulae – II. Anatomy of the ‘thin-shell’ evolution;Monthly Notices of the Royal Astronomical Society;2023-01-14
5. LHAASO J2226+6057 as a pulsar wind nebula;Astronomy & Astrophysics;2022-11-29
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