English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

The powerful wind-wind collision in massive star binaries creates a region ofhigh temperature plasma and accelerates particles to relativistic energies. Ibriefly summarize the hydrodynamics of the wind-wind interaction and theobservational evidence, including recent $\gamma$-ray detections, ofnon-thermal emission from such systems. I then discuss existing models of thenon-thermal emission and their application to date, before concluding with somefuture prospects.

Models of the non-thermal emission from early-type binaries