2016/01/01 by Simon Casassus · 2 citations
Physics and Astronomy · #Accretion (finance) #Accretion disc #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Context (archaeology) #Electrical and Electromagnetic Research #Protoplanetary disk #Quasar #Stars #astro-ph.EP #astro-ph.SR
paper · pdf · doi:10.1017/pasa.2016.7
15 pages, 12 figures, accepted for publication in PASA as a review for the special issue on "Disc dynamics and planet formation"
openalex publication_date 2016/01/01 · openalex created_date 2016/06/24 · arxiv created 2019/05/06 · arxiv updated 2019/05/07 · openalex updated_date 2026/08/05
Abstract Resolved observations are bringing new constraints on the origin of radial gaps in protoplanetary disks. The kinematics, sampled in detail in one case-study, are indicative of non-Keplerian flows, corresponding to warped structures and accretion which may both play a role in the development of cavities. Disk asymmetries seen in the radio continuum are being interpreted in the context of dust segregation via aerodynamic trapping. We summarise recent observational progress, and describe prospects for improvements in the near term.