Debris disks: structure, composition, and variability

AM Hughes, G Duchêne… - Annual Review of …, 2018 - annualreviews.org
Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …

The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model

T Birnstiel, CP Dullemond, Z Zhu… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) is the largest
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …

The size of monomers of dust aggregates in planet-forming disks-Insights from quantitative optical and near-infrared polarimetry

R Tazaki, C Dominik - Astronomy & Astrophysics, 2022 - aanda.org
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 …

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 …

Fractal aggregates of submicron-sized grains in the young planet-forming disk around IM lup

R Tazaki, C Ginski, C Dominik - The Astrophysical Journal …, 2023 - iopscience.iop.org
Despite rapidly growing disk observations, it remains a mystery what primordial dust
aggregates look like and what the physical and chemical properties of their constituent …

A large population study of protoplanetary disks-Explaining the millimeter size-luminosity relation with or without substructure

A Zormpas, T Birnstiel, GP Rosotti… - Astronomy & …, 2022 - aanda.org
Recent subarcsecond resolution surveys of the dust continuum emission from nearby
protoplanetary disks show a strong correlation between the sizes and luminosities of the …

A close-up view of the young circumbinary disk HD 142527

Y Boehler, E Weaver, A Isella, L Ricci… - The Astrophysical …, 2017 - iopscience.iop.org
We present ALMA observations of the 0.88 millimeter dust continuum and the 13 CO and C
18 OJ= 3-2 line emission of the circumbinary disk HD 142527 at a spatial resolution of∼ 0 …

Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk

S Zhang, Z Zhu, T Ueda, A Kataoka… - The Astrophysical …, 2023 - iopscience.iop.org
Dust particle sizes constrained from dust continuum and polarization observations by radio
interferometry are inconsistent by at least an order of magnitude. Motivated by porous dust …

Submillimeter polarization observation of the protoplanetary disk around HD 142527

A Kataoka, T Tsukagoshi, M Momose… - The Astrophysical …, 2016 - iopscience.iop.org
We present the polarization observations toward the circumstellar disk around HD 142527
by using Atacama Large Millimeter/submillimeter Array at the frequency of 343 GHz. The …

Shaking-induced aggregation and flotation in immunoglobulin dispersions: Differences between water and water–ethanol mixtures

NF Bunkin, AV Shkirin, BW Ninham, SN Chirikov… - ACS …, 2020 - ACS Publications
Structural characterization by three complementary methods of laser diagnostics (dynamic
light scattering, laser phase microscopy, and laser polarimetric scatterometry) has …