Warm dust surface chemistry in protoplanetary disks
نویسندگان
چکیده
منابع مشابه
Dust in Protoplanetary Disks
We critically examine the best lines of evidence for grain growth in protoplanetary disks, based on modelling of observed spectral energy distributions and images of T Tauri and Herbig Ae stars. The data are consistent with millimeter-sized grains near disk midplanes, and micron-sized grains near disk surfaces. We review three channels by which grains can grow, including direct condensation fro...
متن کاملChemistry in protoplanetary disks.
3 Material Inventory and Fundamental Chemical Processes in Disks 14 3.1 Inventory of Gas-Phase Molecules . . . . . . . . . . . . . . . . . . . . . . . . . . 14 3.1.1 Results from (Sub-)millimeter Spectroscopy . . . . . . . . . . . . . . . . . 15 3.1.2 Results from Far-Infrared Spectroscopy . . . . . . . . . . . . . . . . . . . 17 3.1.3 Results from Midand Near-Infrared Spectroscopy . . . . . . ...
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We have investigated molecular distributions in protoplanetary disks, adopting a disk model with a temperature gradient in the vertical direction. The model produces sufficiently high abundances of gaseous CO and HCO to account for line observations of T Tauri stars using a sticking probability of unity and without assuming any non-thermal desorption. In regions of radius R ∼> 10 AU, with which...
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The time evolution of dust particles in circumstellar disk-like structures around protostars and young stellar objects was investigated. For the first time, we coupled the dust evolution directly to the evolution of the disk and followed the influence of opacity changes due to collisional aggregation on the dynamics of the disk. For that purpose, we numerically simulated the dynamical evolution...
متن کاملA submillimeter view of protoplanetary dust disks
We present some results from our submillimeter single-dish and aperture synthesis imaging surveys of protoplanetary disks using the JCMT, CSO, and Submillimeter Array (SMA) on Mauna Kea, Hawaii. Employing a simple disk model, we simultaneously fit the spectral energy distributions and spatially resolved submillimeter continuum emission from our SMA survey to constrain disk structure properties,...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2020
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201731747