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Cited article:

Nonthermal X-Rays from Pulsation-driven Shocks in Cepheids

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For how long are particles accelerated in shells of recurrent novae?

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Monthly Notices of the Royal Astronomical Society 515 (2) 1644 (2022)
https://doi.org/10.1093/mnras/stac1844

How unique are pulsar wind nebulae models? Implementation of a multi-parameter, automatic fitting for time-dependent spectra

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Journal of High Energy Astrophysics 36 128 (2022)
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Magnetospheric return-current-heated atmospheres of rotation-powered millisecond pulsars

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Astronomy & Astrophysics 641 A15 (2020)
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Effect of the diffusion parameters on the observed γ -ray spectrum of sources and their contribution to the local all-electron spectrum: The EDGE code

R. López-Coto, J. Hahn, S. BenZvi, et al.
Astroparticle Physics 102 1 (2018)
https://doi.org/10.1016/j.astropartphys.2018.04.003

High-energy Emission from Nonrelativistic Radiative Shocks: Application to Gamma-Ray Novae

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The Astrophysical Journal 852 (1) 62 (2018)
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Multi-year X-Ray Variations of Iron-K and Continuum Emissions in the Young Supernova Remnant Cassiopeia A

Toshiki Sato, Yoshitomo Maeda, Aya Bamba, Satoru Katsuda, Yutaka Ohira, Ryo Yamazaki, Kuniaki Masai, Hironori Matsumoto, Makoto Sawada, Yukikatsu Terada, John P. Hughes and Manabu Ishida
The Astrophysical Journal 836 (2) 225 (2017)
https://doi.org/10.3847/1538-4357/836/2/225

Time-dependent modelling of pulsar wind nebulae: study on the impact of the diffusion-loss approximations

Jonatan Martín, Diego F. Torres and Nanda Rea
Monthly Notices of the Royal Astronomical Society 427 (1) 415 (2012)
https://doi.org/10.1111/j.1365-2966.2012.22014.x