activity
20052018
most citedThermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

494 citations · 951 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2018★ 55 cited

Near-Infrared High-Resolution Imaging Polarimetry of FU Ori-Type Objects: Towards A Unified Scheme for Low-Mass Protostellar Evolution

Michihiro Takami, Guangwei Fu, Hauyu Baobab Liu +14

We present near-IR imaging polarimetry of five classical FU Ori-type objects (FU Ori, V1057 Cyg, V1515 Cyg, V1735 Cyg, Z CMa) with a 0\farcs1 resolution observed using HiCIAO…

astro-ph.SR2016★ 16 cited

Evolution of binary seeds in collapsing protostellar gas clouds

Tatsuya Satsuka, Toru Tsuribe, Suguru Tanaka +1

We perform three dimensional smoothed particle hydrodynamics (SPH) simulations of gas accretion onto the seeds of binary stars to investigate their short-term evolution. Our simula…

astro-ph.SR2016★ 90 cited

Circumstellar Disks of the Most Vigorously Accreting Young Stars

Hauyu Baobab Liu, Michihiro Takami, Tomoyuki Kudo +11

Young stellar objects (YSOs) may not accumulate their mass steadily, as was previously thought, but in a series of violent events manifesting themselves as sharp stellar brightenin…

astro-ph.SR2014★ 8 cited

The Role for the Inner Disk in Mass Accretion to the Star in the Early Phase of Star Formation

Takuya Ohtani, Shigeo S. Kimura, Toru Tsuribe +1

A physical mechanism that drives FU Orionis-type outbursts is reconsidered. We study the effect of inner part of a circumstellar disk covering a region from near the central star t…

astro-ph.EP2013★ 3 cited

Kelvin-Helmholtz Instabilities in Multi-Sized Dust Layers

Yukihiko Hasegawa, Toru Tsuribe

We examine the effect of the dust size distribution on Kelvin-Helmholtz instabilities in the protoplanetary disk with dust sedimentation. With newly taking into account the dust si…

astro-ph.EP2013★ 3 cited

Growth of a Protostar and a Young Circumstellar Disk with High Mass Accretion Rate onto the Disk

Takuya Ohtani, Toru Tsuribe

The growing process of both a young protostar and a circumstellar disk is investigated. Viscous evolution of a disk around a single star is considered with a model where a disk inc…