Dust growth and evolution in protoplanetary disks

T Birnstiel - Annual Review of Astronomy and Astrophysics, 2024 - annualreviews.org
Over the past decade, advancement of observational capabilities, specifically the Atacama
Large Millimeter/submillimeter Array (ALMA) and Spectro-Polarimetric High-contrast …

Dust evolution and the formation of planetesimals

T Birnstiel, M Fang, A Johansen - Space Science Reviews, 2016 - Springer
The solid content of circumstellar disks is inherited from the interstellar medium: dust
particles of at most a micrometer in size. Protoplanetary disks are the environment where …

Early Planet Formation in Embedded Disks (eDisk). I. Overview of the Program and First Results

N Ohashi, JJ Tobin, JK Jørgensen… - The Astrophysical …, 2023 - iopscience.iop.org
We present an overview of the Large Program," Early Planet Formation in Embedded Disks
(eDisk)," conducted with the Atacama Large Millimeter/submillimeter Array (ALMA). The …

The disk substructures at high angular resolution project (DSHARP). I. Motivation, sample, calibration, and overview

SM Andrews, J Huang, LM Pérez, A Isella… - The Astrophysical …, 2018 - iopscience.iop.org
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 …

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70

M Keppler, M Benisty, A Müller, T Henning… - Astronomy & …, 2018 - aanda.org
Context. Young circumstellar disks are the birthplaces of planets. Their study is of prime
interest to understand the physical and chemical conditions under which planet formation …

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 …

Dust masses of young disks: constraining the initial solid reservoir for planet formation

Ł Tychoniec, CF Manara, GP Rosotti… - Astronomy & …, 2020 - aanda.org
Context. Recent years have seen building evidence that planet formation starts early, in the
first~ 0.5 Myr. Studying the dust masses available in young disks enables us to understand …

[HTML][HTML] Photodissociation and photoionisation of atoms and molecules of astrophysical interest

AN Heays, AD Bosman, EF Van Dishoeck - Astronomy & Astrophysics, 2017 - aanda.org
A new collection of photodissociation and photoionisation cross sections for 102 atoms and
molecules of astrochemical interest has been assembled, along with a brief review of the …

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 …

The disk substructures at high angular resolution project (DSHARP). VII. The planet–disk interactions interpretation

S Zhang, Z Zhu, J Huang, VV Guzmán… - The Astrophysical …, 2018 - iopscience.iop.org
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 …