Dusty vortices in protoplanetary disks

S. Inaba*, P. Barge

*この研究の対応する著者

研究成果: Article査読

54 被引用数 (Scopus)

抄録

Global two-dimensional simulations are used to study the coupled evolution of gas and solid particles in a Rossby unstable protoplanetary disk. The initial radial bump in density is unstable to the formation of Rossby waves, which roll up and break into anticyclonic vortices that gradually merge into a large-scale vortical structure persisting for more than 100 rotations. Conditions for the growth of such vortices may naturally appear at the outer edge of the "dead zone" of a protoplanetary disk where gas tends to pile up. We find that solid particles are captured by the vortices and change the evolution: (1) large particles rapidly sink toward the center of the vortices and increase the solid-to-gas ratio by an order of magnitude, (2) solid particles tend to reduce the lifetime of the vortices, and (3) solid particles are effectively confined in the vortices before they are dispersed by the Keplerian shear flow. These results confirm that in a minimum mass solar nebula, persistent vortices could be good places for the formation of the planetesimals or the rocky cores of gas giant planets as soon as particles reach boulder size.

本文言語English
ページ(範囲)415-427
ページ数13
ジャーナルAstrophysical Journal
649
1 I
DOI
出版ステータスPublished - 2006 9月 20

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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