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Cited article:

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Dust Particles in Space: Opportunities for Experimental Research

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Formulating Compressive Strength of Dust Aggregates from Low to High Volume Filling Factors with Numerical Simulations

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Collisional Growth and Fragmentation of Dust Aggregates. II. Mass Distribution of Icy Fragments

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Monte Carlo Simulation of Dust Particles in a Protoplanetary Disk: Crystalline to Amorphous Silicate Ratio in Comets

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Impacts of Viscous Dissipation on Collisional Growth and Fragmentation of Dust Aggregates

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Effective dust growth in laminar circumplanetary discs with magnetic wind-driven accretion

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Dust coagulation and fragmentation in a collapsing cloud core and their influence on non-ideal magnetohydrodynamic effects

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Monthly Notices of the Royal Astronomical Society 515 (2) 2072 (2022)
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Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. II. Dust-ring Formation Mediated by Backreaction and Fragmentation

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Dust Grains Cannot Grow to Millimeter Sizes in Protostellar Envelopes

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Vertical settling of pebbles in turbulent circumbinary discs and the in situ formation of circumbinary planets

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“Ashfall” Induced by Molecular Outflow in Protostar Evolution

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Collisions between micro-sized aggregates: role of porosity, mass ratio, and impact velocity

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Molecules with ALMA at Planet-forming Scales (MAPS). I. Program Overview and Highlights

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Formation of “Blanets” from Dust Grains around the Supermassive Black Holes in Galaxies

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Estimate on Dust Scale Height from the ALMA Dust Continuum Image of the HD 163296 Protoplanetary Disk

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Evolution of dust porosity through coagulation and shattering in the interstellar medium

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X-ray-induced chemistry of water and related molecules in low-mass protostellar envelopes

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Effects of the Compressibility of Turbulence on the Dust Coagulation Process in Protoplanetary Disks

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New Growth Mechanism of Dust Grains in Protoplanetary Disks with Magnetically Driven Disk Winds

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Scattering Polarization of 3 μm Water-ice Feature by Large Icy Grains

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Coagulation Instability in Protoplanetary Disks: A Novel Mechanism Connecting Collisional Growth and Hydrodynamical Clumping of Dust Particles

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The Astrophysical Journal 923 (1) 34 (2021)
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The Water-ice Feature in Near-infrared Disk-scattered Light around HD 142527: Micron-sized Icy Grains Lifted up to the Disk Surface?

Ryo Tazaki, Koji Murakawa, Takayuki Muto, Mitsuhiko Honda and Akio K. Inoue
The Astrophysical Journal 921 (2) 173 (2021)
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Rapid Formation of Gas-giant Planets via Collisional Coagulation from Dust Grains to Planetary Cores

Hiroshi Kobayashi and Hidekazu Tanaka
The Astrophysical Journal 922 (1) 16 (2021)
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Collisional Growth and Fragmentation of Dust Aggregates with Low Mass Ratios. I. Critical Collision Velocity for Water Ice

Yukihiko Hasegawa, Takeru K. Suzuki, Hidekazu Tanaka, Hiroshi Kobayashi and Koji Wada
The Astrophysical Journal 915 (1) 22 (2021)
https://doi.org/10.3847/1538-4357/abf6cf

Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation

Yayaati Chachan, Eve J. Lee and Heather A. Knutson
The Astrophysical Journal 919 (1) 63 (2021)
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Ring Formation by Coagulation of Dust Aggregates in the Early Phase of Disk Evolution around a Protostar

Satoshi Ohashi, Hiroshi Kobayashi, Riouhei Nakatani, Satoshi Okuzumi, Hidekazu Tanaka, Koji Murakawa, Yichen Zhang, Hauyu Baobab Liu and Nami Sakai
The Astrophysical Journal 907 (2) 80 (2021)
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Effect of luminosity outbursts on protoplanetary disk dynamics

Eduard I. Vorobyov, Vardan G. Elbakyan, Michihiro Takami and Hauyu B. Liu
Astronomy & Astrophysics 643 A13 (2020)
https://doi.org/10.1051/0004-6361/202038122

Gravitoviscous protoplanetary disks with a dust component

Vardan G. Elbakyan, Anders Johansen, Michiel Lambrechts, Vitaly Akimkin and Eduard I. Vorobyov
Astronomy & Astrophysics 637 A5 (2020)
https://doi.org/10.1051/0004-6361/201937198

Rapid elimination of small dust grains in molecular clouds

Kedron Silsbee, Alexei V. Ivlev, Olli Sipilä, Paola Caselli and Bo Zhao
Astronomy & Astrophysics 641 A39 (2020)
https://doi.org/10.1051/0004-6361/202038063

Is water ice an efficient facilitator for dust coagulation?

Hiroshi Kimura, Koji Wada, Hiroshi Kobayashi, et al.
Monthly Notices of the Royal Astronomical Society 498 (2) 1801 (2020)
https://doi.org/10.1093/mnras/staa2467

Composition and Size Dependent Sorting in Preplanetary Growth: Seeding the Formation of Mercury-like Planets

Maximilian Kruss and Gerhard Wurm
The Planetary Science Journal 1 (1) 23 (2020)
https://doi.org/10.3847/PSJ/ab93c4

Scattering-induced Intensity Reduction: Large Mass Content with Small Grains in the Inner Region of the TW Hya disk

Takahiro Ueda, Akimasa Kataoka and Takashi Tsukagoshi
The Astrophysical Journal 893 (2) 125 (2020)
https://doi.org/10.3847/1538-4357/ab8223

Size and density sorting of dust grains in SPH simulations of protoplanetary discs – II. Fragmentation

F C Pignatale, J-F Gonzalez, Bernard Bourdon and Caroline Fitoussi
Monthly Notices of the Royal Astronomical Society 490 (3) 4428 (2019)
https://doi.org/10.1093/mnras/stz2883

Dust Pileup at the Dead-zone Inner Edge and Implications for the Disk Shadow

Takahiro Ueda, Mario Flock and Satoshi Okuzumi
The Astrophysical Journal 871 (1) 10 (2019)
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Tracking Dust Grains during Transport and Growth in Protoplanetary Disks

William Misener, Sebastiaan Krijt and Fred J. Ciesla
The Astrophysical Journal 885 (2) 118 (2019)
https://doi.org/10.3847/1538-4357/ab4a13

The Galilean Satellites Formed Slowly from Pebbles

Yuhito Shibaike, Chris W. Ormel, Shigeru Ida, Satoshi Okuzumi and Takanori Sasaki
The Astrophysical Journal 885 (1) 79 (2019)
https://doi.org/10.3847/1538-4357/ab46a7

Nonsticky Ice at the Origin of the Uniformly Polarized Submillimeter Emission from the HL Tau Disk

Satoshi Okuzumi and Ryo Tazaki
The Astrophysical Journal 878 (2) 132 (2019)
https://doi.org/10.3847/1538-4357/ab204d

Pebble accretion in Class 0/I YSOs as a possible pathway for early planet formation

Yuki A Tanaka and Yusuke Tsukamoto
Monthly Notices of the Royal Astronomical Society 484 (2) 1574 (2019)
https://doi.org/10.1093/mnras/stz069

Planetesimal formation in an evolving protoplanetary disk with a dead zone

Sébastien Charnoz, Francesco C. Pignatale, Ryuki Hyodo, et al.
Astronomy & Astrophysics 627 A50 (2019)
https://doi.org/10.1051/0004-6361/201833216

Dust Coagulation Regulated by Turbulent Clustering in Protoplanetary Disks

Takashi Ishihara, Naoki Kobayashi, Kei Enohata, Masayuki Umemura and Kenji Shiraishi
The Astrophysical Journal 854 (2) 81 (2018)
https://doi.org/10.3847/1538-4357/aaa976

Debris disc constraints on planetesimal formation

Alexander V Krivov, Aljoscha Ide, Torsten Löhne, Anders Johansen and Jürgen Blum
Monthly Notices of the Royal Astronomical Society 474 (2) 2564 (2018)
https://doi.org/10.1093/mnras/stx2932

Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift

Sebastiaan Krijt, Kamber R. Schwarz, Edwin A. Bergin and Fred J. Ciesla
The Astrophysical Journal 864 (1) 78 (2018)
https://doi.org/10.3847/1538-4357/aad69b