Numerical Simulation of Dust Circulation in Protoplanetary Disks

被引:0
作者
Fujiwara, Daisuke [1 ]
Watanabe, Sei-ichiro [1 ]
机构
[1] Nagoya Univ, Dept Earth & Planetary Sci, Chikusa Ku, Nagoya, Aichi 4648601, Japan
来源
EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY | 2009年 / 1158卷
关键词
instabilities; protoplanetary disks; solar system: formation; SCHEME;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We numerically simulated the radiation-pressure-induced dust circulation in a protoplanetary disk with a puffed-up turbulent inner rim, and find that dust accumulates in the inner region of the disk.
引用
收藏
页码:123 / 124
页数:2
相关论文
共 4 条
  • [1] Passive irradiated circumstellar disks with an inner hole
    Dullemond, CP
    Dominik, C
    Natta, A
    [J]. ASTROPHYSICAL JOURNAL, 2001, 560 (02) : 957 - 969
  • [2] Exactly conservative semi-Lagrangian scheme for multi-dimensional hyperbolic equations with directional splitting technique
    Nakamura, T
    Tanaka, R
    Yabe, T
    Takizawa, K
    [J]. JOURNAL OF COMPUTATIONAL PHYSICS, 2001, 174 (01) : 171 - 207
  • [3] Surface outflow in optically thick dust disks by radiation pressure
    Takeuchi, T
    Lin, DNC
    [J]. ASTROPHYSICAL JOURNAL, 2003, 593 (01) : 524 - 533
  • [4] Constructing a multi-dimensional oscillation preventing scheme for the advection equation by a rational function
    Xiao, F
    Yabe, T
    Nizam, G
    Ito, T
    [J]. COMPUTER PHYSICS COMMUNICATIONS, 1996, 94 (2-3) : 103 - 118