Gaps, rings, and non-axisymmetric structures in protoplanetary disks: Emission from large grains

2016/03/16 by J. P. Ruge, M. Flock, S. Wolf +5 · 2 citations
Engineering · Physics and Astronomy · #Advanced Thermodynamic Systems and Engines #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Brightness #Circumstellar dust #Debris disk #Dust lane #Protoplanetary disk #Radiation pressure #Radiative transfer #Scale height #Thermal #Vortex #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201526616

published as A&A 590, A17 (2016) · accepted for A&A highlights

arxiv created 2016/03/16 · openalex publication_date 2016/03/28 · arxiv updated 2016/05/04 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. Dust grains with sizes around (sub)mm are expected to couple only weakly to the gas motion in regions beyond 10 au of circumstellar disks. In this work, we investigate the influence of the spatial distribution of these grains on the (sub)mm appearance of magnetized protoplanetary disks.

Citations

• Spatially resolved magnetic field structure in the disk of a T Tauri star
• Trapping solids at the inner edge of the dead zone: 3-D global MHD simulations
• Planets opening dust gaps in gas disks
• Flows of gas through a protoplanetary gap
• Mie scattering by ensembles of particles with very large size parameters
• Rossby Wave Instability of Keplerian Accretion Disks
• RESOLVING THE CIRCUMSTELLAR DISK OF HL TAURI AT MILLIMETER WAVELENGTHS
• Planetesimal formation near the snow line in MRI-driven turbulent protoplanetary disks
• Thermal stability of self-gravitating, optically thin accretion disks
• Dust filtration at gap edges: implications for the spectral energy distributions of discs with embedded planets
• THE VLA VIEW OF THE HL TAU DISK: DISK MASS, GRAIN EVOLUTION, AND EARLY PLANET FORMATION
• Standing on the shoulders of giants
• Self-organisation in protoplanetary discs. Global, non-stratified Hall-MHD simulations

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