Ring Structure Formation in Protoplanetary Disks due to the Two-Fluid Secular Gravitational Instability: An Indicator of Dust Concentration (original) (raw)

Preprint typeset using LATEX style emulateapj v. 11/10/09 TWO-COMPONENT SECULAR GRAVITATIONAL INSTABILITY IN A PROTOPLANETARY DISK: A POSSIBLE MECHANISM FOR CREATING RING-LIKE STRUCTURES

Shu-ichiro Inutsuka

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