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 …
History of the solar nebula from meteorite paleomagnetism
We review recent advances in our understanding of magnetism in the solar nebula and
protoplanetary disks (PPDs). We discuss the implications of theory, meteorite …
protoplanetary disks (PPDs). We discuss the implications of theory, meteorite …
Kinematic detection of a planet carving a gap in a protoplanetary disk
We still do not understand how planets form or why extrasolar planetary systems are so
different from our own Solar System. However, the past few years have dramatically …
different from our own Solar System. However, the past few years have dramatically …
Characterizing the dust content of disk substructures in TW Hydrae
E Macías, O Guerra-Alvarado… - Astronomy & …, 2021 - aanda.org
Context. A key piece of information to understand the origin and role of protoplanetary disk
substructures is their dust content. In particular, disk substructures associated with gas …
substructures is their dust content. In particular, disk substructures associated with gas …
Circumbinary, not transitional: on the spiral arms, cavity, shadows, fast radial flows, streamers, and horseshoe in the HD 142527 disc
We present 3D hydrodynamical models of the HD 142527 protoplanetary disc, a bright and
well-studied disc that shows spirals and shadows in scattered light around a 100 au gas …
well-studied disc that shows spirals and shadows in scattered light around a 100 au gas …
The size of monomers of dust aggregates in planet-forming disks-Insights from quantitative optical and near-infrared polarimetry
Context. The size of the constituent particles (monomers) of dust aggregates is one of the
most uncertain parameters directly affecting collisional growth of aggregates in planet …
most uncertain parameters directly affecting collisional growth of aggregates in planet …
The evidence of radio polarization induced by the radiative grain alignment and self-scattering of dust grains in a protoplanetary disk
A Kataoka, T Tsukagoshi, A Pohl, T Muto… - The Astrophysical …, 2017 - iopscience.iop.org
The mechanisms causing millimeter-wave polarization in protoplanetary disks are under
debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk …
debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk …
Radiation hydrodynamical turbulence in protoplanetary disks: Numerical models and observational constraints
M Flock, RP Nelson, NJ Turner… - The Astrophysical …, 2017 - iopscience.iop.org
Planets are born in protostellar disks, which are now observed with enough resolution to
address questions about internal gas flows. Magnetic forces are possibly drivers of the flows …
address questions about internal gas flows. Magnetic forces are possibly drivers of the flows …
Interferometric observations of magnetic fields in forming stars
CLH Hull, Q Zhang - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
The magnetic field is a key ingredient in the recipe of star formation. However, the
importance of the magnetic field in the early stages of the formation of low-and high-mass …
importance of the magnetic field in the early stages of the formation of low-and high-mass …
ALMA observations of polarized emission toward the CW Tau and DG Tau protoplanetary disks: constraints on dust grain growth and settling
F Bacciotti, JM Girart, M Padovani… - The Astrophysical …, 2018 - iopscience.iop.org
We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet
systems, obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) at 870 μm …
systems, obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) at 870 μm …