Ohtsuki Keiji
Ohtsuki Keiji
Verified email at tiger.kobe-u.ac.jp
TitleCited byYear
Accretional evolution of a planetesimal swarm
SJ Weidenschilling, D Spaute, DR Davis, F Marzari, K Ohtsuki
Icarus 128 (2), 429-455, 1997
3231997
Evolution of planetesimal velocities based on three-body orbital integrations and growth of protoplanets
K Ohtsuki, GR Stewart, S Ida
Icarus 155 (2), 436-453, 2002
1172002
Distribution of accreting gas and angular momentum onto circumplanetary disks
T Tanigawa, K Ohtsuki, MN Machida
The Astrophysical Journal 747 (1), 47, 2012
962012
Capture probability of colliding planetesimals: Dynamical constraints on accretion of planets, satellites, and ring particles
K Ohtsuki
Icarus 106 (1), 228-246, 1993
801993
Dynamics of Saturn's dense rings
J Schmidt, K Ohtsuki, N Rappaport, H Salo, F Spahn
Saturn from Cassini-Huygens, 413-458, 2009
592009
Evolution of particle velocity dispersion in a circumplanetary disk due to inelastic collisions and gravitational interactions
K Ohtsuki
Icarus 137 (1), 152-177, 1999
591999
Local N-body simulations for the distribution and evolution of particle velocities in planetary rings
K Ohtsuki, H Emori
The Astronomical Journal 119 (1), 403, 2000
582000
Growth of the Earth in nebular gas
K Ohtsuki, Y Nakagawa, K Nakazawa
Icarus 75 (3), 552-565, 1988
531988
Artificial acceleration in accumulation due to coarse mass-coordinate divisions in numerical simulation
K Ohtsuki, Y Nakagawa, K Nakazawa
Icarus 83 (1), 205-215, 1990
411990
Planetary rotation by accretion of planetesimals with nonuniform spatial distribution formed by the planet's gravitational perturbation
K Ohtsuki, S Ida
Icarus 131 (2), 393-420, 1998
371998
Runaway planetary growth with collision rate in the solar gravitational field
K Ohtsuki, S Ida
Icarus 85 (2), 499-511, 1990
341990
A multilayer model for thermal infrared emission of Saturn's rings: Basic formulation and implications for Earth-based observations
R Morishima, H Salo, K Ohtsuki
Icarus 201 (2), 634-654, 2009
282009
Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object
R Hyodo, S Charnoz, K Ohtsuki, H Genda
Icarus 282, 195-213, 2017
262017
Evolution of random velocities of planetesimals in the course of accretion
K Ohtsuki
Icarus 98 (1), 20-27, 1992
251992
FORMATION OF CENTAURS’RINGS THROUGH THEIR PARTIAL TIDAL DISRUPTION DURING PLANETARY ENCOUNTERS
R Hyodo, S Charnoz, H Genda, K Ohtsuki
The Astrophysical Journal Letters 828 (1), L8, 2016
242016
Origin and evolution of terrestrial planet rotation
JJ Lissauer, L Dones, K Ohtsuki
Origin of the Earth and Moon, 101-112, 2000
242000
High-accuracy statistical simulation of planetary accretion: I. Test of the accuracy by comparison with the solution to the stochastic coagulation equation
S Inaba, H Tanaka, K Ohtsuki, K Nakazawa
Earth, planets and space 51 (3), 205-217, 1999
241999
Planetary accretion in the solar gravitational field
K Ohtsuki, S Ida, Y Nakagawa, K Nakazawa
Protostars and Planets III, 1089-1107, 1993
221993
Collisional disruption of gravitational aggregates in the tidal environment
R Hyodo, K Ohtsuki
The Astrophysical Journal 787 (1), 56, 2014
212014
A multilayer model for thermal infrared emission of Saturn’s rings II: Albedo, spins, and vertical mixing of ring particles inferred from Cassini CIRS
R Morishima, L Spilker, H Salo, K Ohtsuki, N Altobelli, S Pilortz
Icarus 210 (1), 330-345, 2010
202010
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