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

The assembly and architecture of planetary systems strongly depend on thephysical processes governing the evolution and dispersal of protoplanetarydisks. Since Protostars and Planets VI, new observations and theoreticalinsights favor disk winds as being one of those key processes. This chapterprovides a comprehensive review of recent observations probing outflowing gaslaunched over a range of disk radii for a wide range of evolutionary stages,enabling an empirical understanding of how winds evolve. In parallel, we reviewtheoretical advancements in both magnetohydrodynamic and photoevaporative diskwind models and identify predictions that can be confronted with observations.By linking theory and observations we critically assess the role of disk windsin the evolution and dispersal of protoplanetary disks. Finally, we explore theimpact of disk winds on planet formation and evolution and highlighttheoretical work, observations, and critical tests for future progress.

The Role of Disk Winds in the Evolution and Dispersal of Protoplanetary Disks