activity
20142026
most citedRadiative grain alignment in protoplanetary disks: Implications for polarimetric observations

133 citations · 954 across the 35 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.GA2019★ 6 cited

Distortion of Magnetic Fields in the Dense Core CB81 (L1774, Pipe 42) in the Pipe Nebula

Ryo Kandori, Motohide Tamura, Masao Saito +9

The detailed magnetic field structure of the starless dense core CB81 (L1774, Pipe 42) in the Pipe Nebula was determined based on near-infrared polarimetric observations of backgro…

astro-ph.GA2019★ 10 cited

Distortion of Magnetic Fields in a Starless Core VI: Application of Flux Freezing Model and Core Formation of FeSt 1-457

Ryo Kandori, Kohji Tomisaka, Masao Saito +9

Observational data for the hourglass-like magnetic field toward the starless dense core FeSt 1-457 were compared with a flux freezing magnetic field model (Myers et al. 2018). Fitt…

astro-ph.GA2019

Distortion of Magnetic Fields in Barnard 68

Ryo Kandori, Motohide Tamura, Masao Saito +8

The magnetic field structure, kinematical stability, and evolutionary status of the starless dense core Barnard 68 (B68) are revealed based on the near-infrared polarimetric observ…

astro-ph.EP2019★ 53 cited

Clouds of Fluffy Aggregates: How They Form in Exoplanetary Atmospheres and Influence Transmission Spectra

Kazumasa Ohno, Satoshi Okuzumi, Ryo Tazaki

Transmission spectrum surveys have suggested the ubiquity of high-altitude clouds in exoplanetary atmospheres. Theoretical studies have investigated the formation processes of the…

astro-ph.EP2019★ 65 cited

Unveiling Dust Aggregate Structure in Protoplanetary Disks by Millimeter-wave Scattering Polarization

Ryo Tazaki, Hidekazu Tanaka, Akimasa Kataoka +2

Dust coagulation in a protoplanetary disk is the first step of planetesimal formation. However, a pathway from dust aggregates to planetesimals remains unclear. Both numerical simu…

astro-ph.EP2019★ 69 cited

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

Satoshi Okuzumi, Ryo Tazaki

Recent (sub)millimeter polarimetric observations toward the young star HL Tau have successfully detected polarization emission from its circumstellar disk. The polarization pattern…

astro-ph.SR2019

Polarization in Disks

Ian Stephens, Zhi-Yun Li, Haifeng Yang +24

Polarized dust emission outside of disks reveal the magnetic field morphology of molecular clouds. Within disks, however, polarized dust emission can arise from very different mech…

astro-ph.EP2019★ 37 cited

Millimeter-wave polarization due to grain alignment by the gas flow in protoplanetary disks

Akimasa Kataoka, Satoshi Okuzumi, Ryo Tazaki

Dust grains emit intrinsic polarized emission if they are elongated and aligned in the same direction. The direction of the grain alignment is determined by external forces, such a…

astro-ph.EP2019★ 60 cited

Effect of dust size and structure on scattered light images of protoplanetary discs

Ryo Tazaki, Hidekazu Tanaka, Takayuki Muto +2

We study scattered light properties of protoplanetary discs at near-infrared wavelengths for various dust size and structure by performing radiative transfer simulations. We show t…