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In this paper we review recent progress in our understanding of the chemical evolution of protoplanetary disks. Current observational constraints and theoretical modeling on the chemical composition o...
Tiny grains such as PAHs have been thought to dramatically reduce the coupling between gas and magnetic fields in weakly ionized gas such as in protoplanetary disks (PPDs) because they provide tremend...
Evolution of protoplanetary discs driven by MHD turbulence and other agents。
Dust Opacity and the Contraction of Protoplanetary Atmospheres。
Global Evolution of Solids in Protoplanetary Disks:a Simple Model。
A Spectrographic Study of the Interacting Eclipsing Binary RY Scuti:An Episode in the Rapid Mass Loss Stage or a Protoplanetary Nebula?

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