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20072026
most citedEffects of Ohmic and ambipolar diffusion on the formation and evolution of the first cores, protostars and circumstellar discs

141 citations · 2k across the 55 of their papers we have counts for

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7 papers · 1 filter

astro-ph.EP2025★ 17 cited

Observationally derived magnetic field strength and 3D components in the HD 142527 disk

Satoshi Ohashi, Takayuki Muto, Yusuke Tsukamoto +5

In protoplanetary disks around young stars, magnetic fields play an important role for disk evolution and planet formation. Polarized thermal emission from magnetically aligned gra…

astro-ph.EP2023★ 7 cited

Cosmic-ray ionization rate versus Dust fraction: Which plays a crucial role in the early evolution of the circumstellar disk?

Yudai Kobayashi, Daisuke Takaishi, Yusuke Tsukamoto

We study the formation and early evolution of young stellar objects (YSOs) using three-dimensional non-ideal magnetohydrodynamic (MHD) simulations to investigate the effect of cosm…

astro-ph.EP2021

A new formation scenario of a counter-rotating circumstellar disk: spiral-arm accretion from a circumbinary disk in a triple protostar system

Daisuke Takaishi, Yusuke Tsukamoto, Yasushi Suto

We present the evolution of rotational directions of circumstellar disks in a triple protostar system simulated from a turbulent molecular cloud core with no magnetic field. We fin…

astro-ph.EP2020★ 9 cited

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

Keiichi Wada, Yusuke Tsukamoto, Eiichiro Kokubo

In Wada, Tsukamoto, and Kokubo (2019), we proposed for the first time that a new class of planets, "blanets" (i.e., black hole planets), can be formed around supermassive black hol…

astro-ph.EP2020★ 31 cited

Star-disk alignment in the protoplanetary disks: SPH simulation of the collapse of turbulent molecular cloud cores

Daisuke Takaishi, Yusuke Tsukamoto, Yasushi Suto

We perform a series of three-dimensional smoothed particle hydrodynamics (SPH) simulations to study the evolution of the angle between the protostellar spin and the protoplanetary…

astro-ph.EP2019★ 22 cited

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

Yuki A. Tanaka, Yusuke Tsukamoto

Recent theoretical works suggest that the pebble accretion process is important for planet formation in protoplanetary disks, because it accelerates the growth of planetary cores.…

astro-ph.EP2011★ 2 cited

The self gravity effect on the orbital stability of Twotinos

Yusuke Tsukamoto

We investigate how the self gravity changes the orbital stability of Twotinos using N-body simulations in which the gravitational interaction between planetesimals are fully calcul…