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 Plus annual

Presents the access of premium content as premium feature

Premium Content

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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Gamma-ray binaries are a new class of binary systems, discovered over the last few decades due to the progress made in gamma-ray astronomy. These sources are characterised by spectral energy distributions that are dominated by emission at gamma-ray energies, distinguishing them from other gamma-ray detected binaries. There are currently only six known systems, with a few candidate sources identified. The model most often used to explain these sources is that they consist of a non-accreting pulsar, and that the non-thermal emission originates from the shock which forms between the pulsar and stellar winds. However, a number of questions still remain regarding the exact location and production mechanism behind the emission in these binaries. Here I present a review of gamma-ray binaries, highlighting some recent achievements made, as well as some challenges that still need to be addressed, particular in the era of CTA.

Gamma-ray binaries: binary systems dominated by their gamma-ray emission (Invited Talk)