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 …
Gravitational instabilities in circumstellar disks
Star and planet formation are the complex outcomes of gravitational collapse and angular
momentum transport mediated by protostellar and protoplanetary disks. In this review, we …
momentum transport mediated by protostellar and protoplanetary disks. In this review, we …
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). V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model
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 …
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 …
A steeper than linear disk mass–stellar mass scaling relation
The disk mass is among the most important input parameter for every planet formation
model to determine the number and masses of the planets that can form. We present an …
model to determine the number and masses of the planets that can form. We present an …
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 …
[HTML][HTML] X-shooter spectroscopy of young stellar objects in Lupus-Accretion properties of class II and transitional objects
JM Alcalá, CF Manara, A Natta, A Frasca… - Astronomy & …, 2017 - aanda.org
The mass accretion rate, Ṁ acc, is a key quantity for the understanding of the physical
processes governing the evolution of accretion discs around young low-mass (M⋆≲ 2.0 …
processes governing the evolution of accretion discs around young low-mass (M⋆≲ 2.0 …
Dust and gas in the disk of HL Tauri: surface density, dust settling, and dust-to-gas ratio
C Pinte, WRF Dent, F Ménard, A Hales… - The Astrophysical …, 2015 - iopscience.iop.org
The recent ALMA observations of the disk surrounding HL Tau reveal a very complex dust
spatial distribution. We present a radiative transfer model accounting for the observed gaps …
spatial distribution. We present a radiative transfer model accounting for the observed gaps …
The mass dependence between protoplanetary disks and their stellar hosts
We present a substantial extension of the millimeter (mm) wave continuum photometry
catalog for circumstellar dust disks in the Taurus star-forming region, based on a new" …
catalog for circumstellar dust disks in the Taurus star-forming region, based on a new" …