Accretion Disks Around Young Objects. III. Grain Growth

Abstract

We present detailed models of irradiated T Tauri disks including dust grain growth with power-law size distributions. The models assume complete mixing between dust and gas and solve for the vertical disk structure self-consistentlyincluding the heating effects of stellar irradiation as well as local viscous heating. For a given total dust mass, grain growth is found to decrease the vertical height of the surface where the optical depth to the stellar radiation becomes unit and thus the local irradiation heating, while increasing the disk emission at mm and sub-mm wavelengths. The resulting disk models are less geometrically thick than our previous models assuming interstellar medium dust, and agree better with observed spectral energy distributions and images of edge-on disks, like HK Tau/c and HH 30. The implications of models with grain growth for determining disk masses from long-wavelength emission are considered.

29 pages, including 11 figures and 1 table, APJ accepted

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• Wavelength-Dependent Extinction and Grain Sizes in Dippers
• The Young Stellar Population, Distance, and Cloud-Cloud Collision Induced Star Formation Scenario of the Trifid Nebula
• Exploring the Grain Properties in the Disk of HL Tau with an Evolutionary Model
• The Radial Profile of Dust Grain Size in the Protoplanetary Disk of DS Tau
• Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt
• $R_V$ from multi-waveband galaxy polarimetry in supernovae vicinity
• Planet Formation by Gas-Assisted Accretion of Small Solids
• The Disappearing Envelope around the Transitional Class I Object L43
• The Impact of Silicate Grain Coagulation on Millimeter Emission from Massive Protostellar Disks
• Measuring Dust Masses of Protoplanetary Disks in Serpens and L1641/L1647 with ALMA
• Hidden power of near-infrared data for the study of young clusters: Illustrative case of RCW 38
• Thermally driven spontaneous dust accumulation in the inner regions of protoplanetary disks
• Molecular Line Emission from Accretion Disks Around YSOs
• Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations
• The dispersal of protoplanetary discs -- III: Influence of stellar mass on disc photoevaporation
• "Ashfall" Induced by Molecular Outflow in Protostar Evolution. II. Analytical Study on the Maximum Size of Dust Grains Lifted by Outflows
• Comets in context: Comparing comet compositions with protosolar nebula models
• Revealing magnetic field structure at the surfaces of protoplanetary disks via near-infrared circular polarization
• Ice coverage of dust grains in cold astrophysical environments
• Fine-grained rim formation via kinetic dust aggregation in shock waves around evaporating icy planetesimals