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 …
[HTML][HTML] Empirical constraints on turbulence in proto-planetary discs
GP Rosotti - New Astronomy Reviews, 2023 - Elsevier
Proto-planetary discs, the birth environment of planets, are an example of a structure
commonly found in astrophysics, accretion discs. Identifying the mechanism responsible for …
commonly found in astrophysics, accretion discs. Identifying the mechanism responsible for …
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 …
A highly settled disk around oph163131
M Villenave, KR Stapelfeldt, G Duchêne… - The Astrophysical …, 2022 - iopscience.iop.org
High dust density in the midplane of protoplanetary disks is favorable for efficient grain
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
Contemporary formation of early Solar System planetesimals at two distinct radial locations
The formation of planetesimals is expected to occur via particle-gas instabilities that
concentrate dust into self-gravitating clumps,–. Triggering these instabilities requires the …
concentrate dust into self-gravitating clumps,–. Triggering these instabilities requires 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 …
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 …
Planetesimal rings as the cause of the Solar System's planetary architecture
Astronomical observations reveal that protoplanetary disks around young stars commonly
have ring-and gap-like structures in their dust distributions. These features are associated …
have ring-and gap-like structures in their dust distributions. These features are associated …
Compact disks in a high-resolution ALMA survey of dust structures in the Taurus molecular cloud
We present a high-resolution (∼ 0 farcs 12,∼ 16 au, mean sensitivity of 50 μJy beam− 1 at
225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spectral type …
225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spectral type …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …
classical planet formation theory, developed when the only known planetary system was our …