Modelling accretion in transitional disks

2013/10/30 by Tobias W. A. Müller, Wilhelm Kley · 22 citations
Physics and Astronomy · #Accretion (finance) #Accretion disc #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Clearance #Planet #Planetary system #Scientific Research and Discoveries #Stars #T Tauri star #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201322503

published in Astronomy and Astrophysics 560, A40 (EDP Sciences) · 10 pages, 29 figures, accepted for publication in Astronomy & Astrophysics

openalex publication_date 2013/10/30 · arxiv created 2013/12/02 · arxiv updated 2013/12/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Transitional disks are protoplanetary disks around young stars that display inner holes in the dust distribution within a few au that are accompanied by some gas accretion onto the central star. These cavities could possibly be created by the presence of one or more massive planets that opened a large gap or even cleared the whole inner region.

Citations

• A comparative study of disc-planet interaction
• Disk eccentricity and embedded planets
• Dust filtration at gap edges: implications for the spectral energy distributions of discs with embedded planets

Cited by

• exoALMA XXIII. Estimating Disk and Planet Properties from Dust Morphologies with DBNets2.0
• Variable Accretion onto Protoplanet Host Star PDS 70