Particle acceleration in colliding flows: Binary star winds and other double-shock structures

Mikhail Malkov; Martin Lemoine

doi:10.1103/PhysRevE.107.025201

Journal Articles Physical Review E Year : 2023

Particle acceleration in colliding flows: Binary star winds and other double-shock structures

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Mikhail Malkov

Function : Author
PersonId : 1309481
ORCID : 0000-0001-6360-1987

Martin Lemoine

Function : Author
PersonId : 740762
IdHAL : martin-lemoine
ORCID : 0000-0002-2395-7812
IdRef : 079322816

Institut d'Astrophysique de Paris

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High Energy Astrophysical Phenomena [astro-ph.HE]

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2212.08788.pdf (2.56 Mo)

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https://cnrs.hal.science/hal-04288930

Submitted on : Thursday, November 16, 2023-11:52:29 AM

Last modification on : Thursday, June 20, 2024-8:20:03 AM

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hal-04288930 , version 1 (16-11-2023)

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HAL Id : hal-04288930 , version 1
DOI : 10.1103/PhysRevE.107.025201

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Mikhail Malkov, Martin Lemoine. Particle acceleration in colliding flows: Binary star winds and other double-shock structures. Physical Review E , 2023, 107 (2), pp.025201. ⟨10.1103/PhysRevE.107.025201⟩. ⟨hal-04288930⟩

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Particle acceleration in colliding flows: Binary star winds and other double-shock structures

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