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

Under the assumption that LS 5039 is a system composed by a pulsar rotatingaround an O6.5V star in a $\sim 3.9$ day orbit, we present the results of atheoretical modeling of the high energy phenomenology observed by the HighEnergy Stereoscopy Array (H.E.S.S.). This model (including detailed account ofthe system geometry, Klein-Nishina inverse Compton, $\gamma$-$\gamma$absorption, and cascading) is able to describe well the rich observedphenomenology found in the system at all timescales, both flux andspectrum-wise.

Pulsar model of the high energy phenomenology of LS 5039