Modeling the nonaxisymmetric structure in the HD 163296 disk with planet-disk interaction

Abstract

High resolution ALMA observations revealed a variety of rich substructures in numerous protoplanetary disks. These structures consist of rings, gaps and asymmetric features. It is debated whether planets can be accounted for these substructures in the dust continuum. Characterizing the origin of asymmetries as seen in HD 163296 might lead to a better understanding of planet formation and the underlying physical parameters of the system. We test the possibility of the formation of the crescent-shaped asymmetry in the HD 163296 disk through planet-disk interaction. The goal is to obtain constraints on planet masses and eccentricities and disk viscosities. Two dimensional, multi-fluid, hydrodynamical simulations are performed with the FARGO3D code including three embedded planets. Dust is described with the pressureless fluid approach and is distributed over eight size bins. Resulting grids are post-processed with the radiative transfer code RADMC-3D and the CASA software to model synthetic observations. We find that the crescent-shaped asymmetry can be qualitatively modeled with a Jupiter mass planet at a radial distance of 48 au. Dust is trapped preferably in the trailing Lagrange point L5 with a mass of 10 to 15 earth masses. Increased values of eccentricity of the innermost Jupiter mass planet damages the stability of the crescent-shaped feature and does not reproduce the observed radial proximity to the first prominent ring in the system. Generally, a low level of viscosity ($\alpha \le 2\cdot 10^{-3}$) is necessary to allow the existence of such a feature. Including dust feedback the leading point L4 can dominantly capture dust for dust grains with an initial Stokes number $\le 3.6\cdot 10^{-2}$. The observational results suggest a negligible effect of dust feedback since only one such feature has been detected so far.

arXiv commentAccepted for publication in Astronomy & Astrophysics

References in corpus (66)

• Gaia Data Release 2. Summary of the contents and survey properties
• First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region
• The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
• Planet-disk interaction and orbital evolution
• Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
• Rossby Wave Instability of Keplerian Accretion Disks
• A Major Asymmetric Dust Trap in a Transition Disk
• FARGO: a fast eulerian transport algorithm for differentially rotating disks
• The Disk Substructures at High Angular Resolution Project (DSHARP): II. Characteristics of Annular Substructures
• A comparative study of disc-planet interaction
• Turbulence in Accretion Disks. Vorticity Generation and Angular Momentum Transport via the Global Baroclinic Instability
• The Disk Substructures at High Angular Resolution Project (DSHARP): VII. The Planet-Disk Interactions Interpretation
• The Disk Substructures at High Angular Resolution Project (DSHARP) VI: Dust trapping in thin-ringed protoplanetary disks
• Mass Flow and Accretion through gaps in Accretion Discs
• Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations
• The Disk Substructures at High Angular Resolution Project (DSHARP): V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model
• Radiative Equilibrium and Temperature Correction in Monte Carlo Radiation Transfer
• Rossby Wave Instability of Thin Accretion Disks -- II. Detailed Linear Theory
• A Kinematical Detection of Two Embedded Jupiter Mass Planets in HD 163296
• Observational Signatures of Planets in Protoplanetary Disks I: Gaps Opened by Single and Multiple Young Planets in Disks
• Weak Turbulence in the HD 163296 Protoplanetary Disk Revealed by ALMA CO Observations
• A Three-Dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk using DCO${}^{+}$
• On planet formation in HL Tau
• FARGO3D: A new GPU-oriented MHD code
• Planets opening dust gaps in gas disks
• Accelerated planetesimal growth in self-gravitating protoplanetary discs
• Dust flow in gas disks in the presence of embedded planets
• One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering
• A Spatially Resolved Inner Hole in the Disk around GM Aurigae
• The Disk Substructures at High Angular Resolution Project (DSHARP) - IX. A high definition study of the HD 163296 planet forming disk
• Standing on the shoulders of giants: Trojan Earths and vortex trapping in low mass self-gravitating protoplanetary disks of gas and solids
• Nine localised deviations from Keplerian rotation in the DSHARP circumstellar disks: Kinematic evidence for protoplanets carving the gaps
• Particle Concentration At Planet Induced Gap Edges and Vortices: I. Inviscid 3-D Hydro Disks
• The co-orbital corotation torque in a viscous disk: numerical simulations
• On the formation of multiple concentric rings and gaps in protoplanetary disks
• Treating gravity in thin disk simulations
• The anomalously low (sub)millimeter spectral indices of some protoplanetary disks may be explained by dust self-scattering
• Can dead zones create structures like a transition disk?
• Asymptotically stable numerical method for multispecies momentum transfer: gas and multifluid-dust test suite and implementation in FARGO3D
• Planetesimal formation via fragmentation in self-gravitating protoplanetary discs
• Evidence for a massive dust-trapping vortex connected to spirals: a multi-wavelength analysis of the HD~135344B protoplanetary disk
• Dust unveils the formation of a mini-Neptune planet in a protoplanetary ring
• Characterizing the variable dust permeability of planet-induced gaps
• Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
• Gas and dust hydrodynamical simulations of massive lopsided transition discs - II. Dust concentration
• Scattered light images of spiral arms in marginally gravitationally unstable discs with an embedded planet
• Planet gaps in the dust layer of 3D protoplanetary disks: I. Hydrodynamical simulations of T Tauri disks
• On the accumulation of planetesimals near disc gaps created by protoplanets
• New constraints on turbulence and embedded planet mass in the HD 163296 disk from planet-disk hydrodynamic simulations
• The effect of a planet on the dust distribution in a 3D protoplanetary disk
• Slowly-growing gap-opening planets trigger weaker vortices
• Vortex Formation and Survival in Protoplanetary Disks subject to Vertical Shear Instability
• Migrating super-Earths in low-viscosity discs: unveiling the roles of feedback, vortices, and laminar accretion flows
• Midplane temperature and outer edge of the protoplanetary disk around HD 163296
• How do giant planetary cores shape the dust disk? HL Tau system
• Predicting the observational signature of migrating Neptune-sized planets in low-viscosity disks
• Is the ring inside or outside the planet?: The effect of planet migration on dust rings
• On the planetary interpretation of multiple gaps and rings in protoplanetary disks seen by ALMA
• Impacts of dust feedback on a dust ring induced by a planet in a protoplanetary disk
• Importance of radiative effects in gap opening by planets in protoplanetary disks
• Observational diagnostics of elongated planet-induced vortices with realistic planet formation timescales
• Dust trapping around Lagrangian points in protoplanetary disks
• Rossby Wave Instability and Long-Term Evolution of Dead Zones in Protoplanetary Discs
• Constraining the masses of planets in protoplanetary discs from the presence or absence of vortices -- Comparison with ALMA observations
• Gap Formation in the Dust Layer of 3D Protoplanetary Disks
• Migration jumps of planets in transition disks

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• Modeling planet-induced gaps and rings in ALMA disks: the role of in-plane radiative diffusion
• Millimeter Gap Contrast as a Probe for Turbulence Level in Protoplanetary Disks
• A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain
• Tentative co-orbital submillimeter emission within the Lagrangian region L5 of the protoplanet PDS 70 b
• Extreme Pebble Accretion in Ringed Protoplanetary Discs
• The steady-state hydrodynamics of a long-lived disc: planetary system architecture and prospects of observing a circumplanetary disc shadow in V4046Sgr
• The Morphology of the HD 163296 jet as a window on its planetary system
• Distributions of gas and small and large grains in the LkH$\alpha 330$ disk trace a young planetary system
• Spreading pressure bumps in gas-dust discs can stall planet migration via planet-vortex interactions
• Substructures in protoplanetary disks imprinted by compact planetary systems
• Testing planet formation from the ultraviolet to the millimeter
• Emerging population of gap-opening planets around type-A stars -- Long-term evolution of the forming planets around HD 163296
• Single Fluid vs. Multifluid: Comparison between single fluid and multifluid dust models for disc planet interactions
• Dust traps and gas kinematic signatures in a crescent structure of a planet-forming disk