19 papers found
Refreshing results…
A Multifrequency ALMA Characterization of Substructures in the GM Aur Protoplanetary Disk
The effects of disc self-gravity and radiative cooling on the formation of gaps and spirals by young planets
One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering
The Disk Substructures at High Angular Resolution Project (DSHARP). I. Motivation, Sample, Calibration, and Overview
The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation
The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A High-definition Study of the HD 163296 Planet-forming Disk
The Disk Substructures at High Angular Resolution Project (DSHARP). X. Multiple Rings, a Misaligned Inner Disk, and a Bright Arc in the Disk around the T Tauri star HD 143006
The Disk Substructures at High Angular Resolution Program (DSHARP). VIII. The Rich Ringed Substructures in the AS 209 Disk
The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks
The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA Maps of Protoplanetary Disks in Terms of a Dust Model
The Disk Substructures at High Angular Resolution Project (DSHARP). IV. Characterizing Substructures and Interactions in Disks around Multiple Star Systems
The Disk Substructures at High Angular Resolution Project (DSHARP). III. Spiral Structures in the Millimeter Continuum of the Elias 27, IM Lup, and WaOph 6 Disks
The Disk Substructures at High Angular Resolution Project (DSHARP). II. Characteristics of Annular Substructures
Disk Substructures at High Angular Resolution Program (DSHARP): VIII. The Rich Ringed Substructures in the AS 209 Disk
On estimating angular momenta of infalling protostellar cores from observations
ALMA Observations of the Epoch of Planet Formation
Simulations of star-forming molecular clouds: observational predictions
The Circum-Galactic Medium of Massive Spirals. II. Probing the Nature of Hot Gaseous Halo around the Most Massive Isolated Spiral Galaxies
The Circum-Galactic Medium of MASsive Spirals (CGM-MASS): XMM-Newton observations of the hot CGM
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