Volume 354 -
High Energy Phenomena in Relativistic Outflows VII (HEPRO VII) -
Relativistic outflows from extragalactic sources
On the interaction of pulsar winds and clumpy stellar winds
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Published on:
February 25, 2020
Abstract
High-mass binaries hosting a non-accreting pulsar are sources of gamma rays, which are thought to originate in the wind-wind collision region. The stellar wind is expected to be clumpy, which could have important effects on the emitting flow dynamics, and thus on the associated non-thermal radiation. We adopt here a combination of Monte-Carlo and semi-analytical hydrodynamic calculations to explore the impact of clumps on the shocked wind structure on the scales of the binary system.
DOI: https://doi.org/10.22323/1.354.0031
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.