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 …
Molecules with ALMA at Planet-forming Scales (MAPS). I. Program overview and highlights
Planets form and obtain their compositions in dust-and gas-rich disks around young stars,
and the outcome of this process is intimately linked to the disk chemical properties. The …
and the outcome of this process is intimately linked to the disk chemical properties. The …
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 …
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 …
Bifurcation of planetary building blocks during Solar System formation
T Lichtenberg, J Dra̧żkowska, M Schönbächler… - Science, 2021 - science.org
Geochemical and astronomical evidence demonstrates that planet formation occurred in two
spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We …
spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We …
ALMA survey of lupus protoplanetary disks. II. Gas disk radii
Abstract We present Atacama Large Millimeter/Sub-Millimeter Array (ALMA) Band 6
observations of a complete sample of protoplanetary disks in the young (∼ 1–3 Myr) Lupus …
observations of a complete sample of protoplanetary disks in the young (∼ 1–3 Myr) Lupus …
A kinematical detection of two embedded Jupiter-mass planets in HD 163296
We present the first kinematical detection of embedded protoplanets within a protoplanetary
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
Kinematic evidence for an embedded protoplanet in a circumstellar disk
Disks of gas and dust surrounding young stars are the birthplace of planets. However, the
direct detection of protoplanets forming within disks has proved elusive to date. We present …
direct detection of protoplanets forming within disks has proved elusive to date. We present …
Accretion onto pre-main-sequence stars
L Hartmann, G Herczeg, N Calvet - Annual Review of Astronomy …, 2016 - annualreviews.org
Accretion through circumstellar disks plays an important role in star formation and in
establishing the properties of the regions in which planets form and migrate. The …
establishing the properties of the regions in which planets form and migrate. The …