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

We consider the pulsar rotation assuming that the neutron star consists ofcrust component (which rotation is observed) and two core components. One ofthe core components contains pinned superfluid which can, for some reasons,suddenly inject small fraction of stored angular momentum in it. In theframework of this simple model the star can demonstrate glitch-like eventstogether with long period precession (with period $1-10^{4}$ years).

Precession and glitches in the framework of three-component model of neutron star