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Paper: Diagnosing Gas Dispersal Processes in Protoplanetary Disks
Volume: 476, New Trends in Radio Astronomy in the ALMA Era
Page: 209
Authors: Nomura, H.; Walsh, C.; Millar, T. J.; Aikawa, Y.
Abstract: ALMA observations with high spatial resolution and high sensitivity will reveal detailed structure of planet forming regions in protoplanetary disks. In advance of this ALMA era, we have modelled physical and chemical structure and line emission from disks to study how molecular lines can be useful for diagnosing gas dispersal processes such as magnetorotational instability and photoevaporation.
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