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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Many members of nearby young moving groups exhibit infrared excess attributedto circumstellar debris dust, formed via erosion of planetesimals. With theirproximity and well-dated ages, these groups are excellent laboratories forstudying the early evolution of debris dust and of planetesimal belts. ALMA canspatially resolve the disk emission, revealing the location and extent of thesebelts, putting constraints on planetesimal evolution models, and allowing us tostudy planet-disk interactions. While the main trends of dust evolution indebris disks are well-known, there is almost no information on the evolution ofgas. During the transition from protoplanetary to debris state, even the originof gas is dubious. Here we review the exciting new results ALMA provided byobserving young debris disks, and discuss possible future research directions.

Debris Disks in Nearby Young Moving Groups in the ALMA Era