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 Plus

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

Zendy Tools

Zendy Open

In our own solar system, the necessity of understanding space weather isreadily evident. Fortunately for Earth, our nearest stellar neighbor isrelatively quiet, exhibiting activity levels several orders of magnitude lowerthan young, solar-type stars. In protoplanetary systems, stellar magneticphenomena observed are analogous to the solar case, but dramatically enhancedon all physical scales: bigger, more energetic, more frequent. While coronalmass ejections (CMEs) could play a significant role in the evolution ofprotoplanets, they could also affect the evolution of the central star itself.To assess the consequences of prominence eruption/CMEs, we have invoked thesolar-stellar connection to estimate, for young, solar-type stars, howfrequently stellar CMEs may occur and their attendant mass and angular momentumloss rates. We will demonstrate the necessary conditions under which CMEs couldslow stellar rotation.

Coronal Mass Ejections and Angular Momentum Loss in Young Stars