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 …
The dispersal of planet-forming discs: theory confronts observations
B Ercolano, I Pascucci - Royal Society Open Science, 2017 - royalsocietypublishing.org
Discs of gas and dust around million-year-old stars are a by-product of the star formation
process and provide the raw material to form planets. Hence, their evolution and dispersal …
process and provide the raw material to form planets. Hence, their evolution and dispersal …
Images of embedded Jovian planet formation at a wide separation around AB Aurigae
Direct images of protoplanets embedded in disks around infant stars provide the key to
understanding the formation of gas giant planets such as Jupiter. Using the Subaru …
understanding the formation of gas giant planets such as Jupiter. Using the Subaru …
The disk substructures at high angular resolution project (DSHARP). I. Motivation, sample, calibration, and overview
Abstract We introduce the Disk Substructures at High Angular Resolution Project (DSHARP),
one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …
one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …
Two accreting protoplanets around the young star PDS 70
Newly forming protoplanets are expected to create cavities and substructures in young, gas-
rich protoplanetary disks,–, but they are difficult to detect as they could be confused with disk …
rich protoplanetary disks,–, but they are difficult to detect as they could be confused with disk …
Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region
Rings are the most frequently revealed substructure in Atacama Large Millimeter/
submillimeter Array (ALMA) dust observations of protoplanetary disks, but their origin is still …
submillimeter Array (ALMA) dust observations of protoplanetary disks, but their origin is still …
The disk substructures at high angular resolution project (DSHARP). VI. Dust trap** in thin-ringed protoplanetary disks
CP Dullemond, T Birnstiel, J Huang… - The Astrophysical …, 2018 - iopscience.iop.org
A large fraction of the protoplanetary disks observed with ALMA display multiple well-
defined and nearly perfectly circular rings in the continuum, in many cases with substantial …
defined and nearly perfectly circular rings in the continuum, in many cases with substantial …
The disk substructures at high angular resolution project (DSHARP). II. Characteristics of annular substructures
J Huang, SM Andrews, CP Dullemond… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) used ALMA
to map the 1.25 mm continuum of protoplanetary disks at a spatial resolution of∼ 5 au. We …
to map the 1.25 mm continuum of protoplanetary disks at a spatial resolution of∼ 5 au. We …
The disk substructures at high angular resolution project (DSHARP). VII. The planet–disk interactions interpretation
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) provides a
large sample of protoplanetary disks with substructures that could be induced by young …
large sample of protoplanetary disks with substructures that could be induced by young …
Observations of edge-on protoplanetary disks with ALMA-I. Results from continuum data
Aims. We aim to study vertical settling and radial drift of dust in protoplanetary disks from a
different perspective: an edge-on view. An estimation of the amplitude of settling and drift is …
different perspective: an edge-on view. An estimation of the amplitude of settling and drift is …