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/

Zendy Pro

Presents the zaia usage as premium feature

ZAIA

Presents AI Discovery search usage as a premium feature

AI Discovery

Presents AI Discovery explain and summary usage as a premium feature

Content Analysis

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Presents the pdf analysis as premium feature

PDF Analysis

1500 Top-up

3000 Top-up

Zendy Basic

2500 Top-up

Zendy Unlimited

Presents the access of premium content as premium feature

Premium Content

The recent improvement in VLBI arrays is providing information of theemission and magnetic field structure of relativistic jets, both extragalacticand galactic (microquasars), with unprecedented spatial and temporalresolution. These observations are revealing the importance of thehydrodynamical processes that govern the jet evolution, which can be studied bythe recently developed time-dependent relativistic hydrodynamical models.Computation of the non-thermal emission from these hydrodynamical models, andits comparison with actual sources, is proving as one of the most powerfultools in the understanding of the physical processes taking place in thesejets. This paper reviews some of the recent observational results, as well asthe numerical models used to interpret them.

Observations and Simulations of Relativistic Jets