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 …
Planet-disk interaction and orbital evolution
W Kley, RP Nelson - Annual Review of Astronomy and …, 2012 - annualreviews.org
As planets form and grow within gaseous protoplanetary disks, the mutual gravitational
interaction between the disk and planet leads to the exchange of angular momentum and …
interaction between the disk and planet leads to the exchange of angular momentum and …
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 …
Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
P Mollière, T Molyarova, B Bitsch… - The Astrophysical …, 2022 - iopscience.iop.org
Constraining planet formation based on the atmospheric composition of exoplanets is a
fundamental goal of the exoplanet community. Existing studies commonly try to constrain …
fundamental goal of the exoplanet community. Existing studies commonly try to constrain …
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 …
Ringed substructure and a gap at 1 au in the nearest protoplanetary disk
We present long baseline Atacama Large Millimeter/submillimeter Array (ALMA)
observations of the 870 μm continuum emission from the nearest gas-rich protoplanetary …
observations of the 870 μm continuum emission from the nearest gas-rich protoplanetary …
Rapid growth of gas-giant cores by pebble accretion
M Lambrechts, A Johansen - Astronomy & Astrophysics, 2012 - aanda.org
The observed lifetimes of gaseous protoplanetary discs place strong constraints on gas and
ice giant formation in the core accretion scenario. The approximately 10-Earth-mass solid …
ice giant formation in the core accretion scenario. The approximately 10-Earth-mass solid …
Pebble-isolation mass: Scaling law and implications for the formation of super-Earths and gas giants
B Bitsch, A Morbidelli, A Johansen, E Lega… - Astronomy & …, 2018 - aanda.org
The growth of a planetary core by pebble accretion stops at the so-called pebble isolation
mass, when the core generates a pressure bump that traps drifting pebbles outside its orbit …
mass, when the core generates a pressure bump that traps drifting pebbles outside its orbit …
Separating gas-giant and ice-giant planets by halting pebble accretion
M Lambrechts, A Johansen, A Morbidelli - Astronomy & Astrophysics, 2014 - aanda.org
In the solar system giant planets come in two flavours: gas giants (Jupiter and Saturn) with
massive gas envelopes, and ice giants (Uranus and Neptune) with much thinner envelopes …
massive gas envelopes, and ice giants (Uranus and Neptune) with much thinner envelopes …
Sintering-induced dust ring formation in protoplanetary disks: Application to the HL tau disk
The latest observation of HL Tau by ALMA revealed spectacular concentric dust rings in its
circumstellar disk. We attempt to explain the multiple ring structure as a consequence of …
circumstellar disk. We attempt to explain the multiple ring structure as a consequence of …