Colliding-wind binary systems: Diffusive shock acceleration and non-thermal emission

Pittard, JM orcid.org/0000-0003-2244-5070, Vila, GS and Romero, GE (2020) Colliding-wind binary systems: Diffusive shock acceleration and non-thermal emission. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

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Copyright, Publisher and Additional Information: © 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. This is an author produced version of a journal article published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: binaries: general, gamma-rays: stars, radiation mechanisms: non-thermal, stars: early-type, stars: winds, outflows, stars: Wolf-Rayet
Dates:
  • Accepted: 10 April 2020
  • Published (online): 23 April 2020
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 11 May 2020 10:05
Last Modified: 11 May 2020 10:05
Status: Published online
Publisher: Oxford University Press (OUP)
Identification Number: https://doi.org/10.1093/mnras/staa1099

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