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

Most stars have masses similar to that of the Sun and can be expected to burn “slowly” for a billion years or more. About one star in a hundred, however, is considerably more massive than the Sun (perhaps 10M ) and consumes its fuel at a much higher rate, arriving at a spectacular end in the form of a supernova explosion after about 10 million years. Most of the mass of the progenitor star is expelled into space, leaving behind a highly magnetized and rapidly rotating neutron star. Heavier progenitor stars (M > 15M ) completely collapse, forming black holes.

A Lab to Detect Radio Pulsars Using a Remotely Accessed 18-Meter Radiotelescope