Modeling gas-dust interactions in debris disks

dc.contributor.author	Kuchner, Marc	en
dc.contributor.author	Lyra, Wladimir	en
dc.contributor.author	Richert, Alexander J.W.	en
dc.date.accessioned	2017-10-11T21:49:19Z
dc.date.available	2017-10-11T21:49:19Z
dc.date.issued	2017	en
dc.identifier.citation	Bulletin of the American Astronomical Society 49(2). (2017)	en
dc.identifier.other	http://adsabs.harvard.edu/abs/2017AAS...22942002R	en
dc.identifier.uri	http://hdl.handle.net/10211.3/197070	en
dc.description.abstract	The discovery of gas in debris disks has raised the question of whether gas-dust interactions can observably affect global disk structure. This has important implications for identifying planets in debris disks, as well as probing dust grain composition, which is key to understanding the habitability of planetary systems. In this dissertation talk, I present two-dimensional global hydrodynamical models of debris disks with gas and discuss the effects of the gas on the global distribution of the dust.	en
dc.language.iso	en	en
dc.publisher	American Astronomical Society Meeting Abstracts	en
dc.title	Modeling gas-dust interactions in debris disks	en
dc.type	Conference paper or proceedings	en

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