Observations of protoplanetary disk structures
SM Andrews - Annual Review of Astronomy and Astrophysics, 2020 - annualreviews.org
The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …
and planet formation. Their structures, meaning the spatial variations of the disk physical …
Debris disks: structure, composition, and variability
AM Hughes, G Duchêne… - Annual Review of …, 2018 - annualreviews.org
Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …
wide range of ages. Those around main sequence stars are analogous to the Solar System's …
The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model
T Birnstiel, CP Dullemond, Z Zhu… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) is the largest
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …
Sintering-induced dust ring formation in protoplanetary disks: Application to the HL tau disk
The latest observation of HL Tau by ALMA revealed spectacular concentric dust rings in its
circumstellar disk. We attempt to explain the multiple ring structure as a consequence of …
circumstellar disk. We attempt to explain the multiple ring structure as a consequence of …
Consistent dust and gas models for protoplanetary disks-I. Disk shape, dust settling, opacities, and PAHs
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary
disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of …
disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of …
Shadows cast on the transition disk of hd 135344b-multiwavelength vlt/sphere polarimetric differential imaging
Context. The protoplanetary disk around the F-type star HD 135344B (SAO 206462) is in a
transition stage and shows many intriguing structures both in scattered light and thermal …
transition stage and shows many intriguing structures both in scattered light and thermal …
The size of monomers of dust aggregates in planet-forming disks-Insights from quantitative optical and near-infrared polarimetry
Context. The size of the constituent particles (monomers) of dust aggregates is one of the
most uncertain parameters directly affecting collisional growth of aggregates in planet …
most uncertain parameters directly affecting collisional growth of aggregates in planet …
The evidence of radio polarization induced by the radiative grain alignment and self-scattering of dust grains in a protoplanetary disk
A Kataoka, T Tsukagoshi, A Pohl, T Muto… - The Astrophysical …, 2017 - iopscience.iop.org
The mechanisms causing millimeter-wave polarization in protoplanetary disks are under
debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk …
debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk …
Grain-size measurements in protoplanetary disks indicate fragile pebbles and low turbulence
Context. Constraining the turbulence level and pebble size in protoplanetary disks is an
essential initial step in understanding the aerodynamic properties of pebbles, which are …
essential initial step in understanding the aerodynamic properties of pebbles, which are …
Near-infrared scattered light properties of the HR 4796 A dust ring-A measured scattering phase function from 13.6° to 166.6°
Context. HR 4796 A is surrounded by a debris disc, observed in scattered light as an
inclined ring with a high surface brightness. Past observations have raised several …
inclined ring with a high surface brightness. Past observations have raised several …