The Inner 25 au Debris Distribution in the ϵ Eri System

The Inner 25 au Debris Distribution in the ϵ Eri System

Debris disk morphology is wavelength dependent due to the wide range of particle sizes and size-dependent dynamics influenced by various forces. Resolved images of nearby debris disks reveal complex disk structures that are difficult to distinguish from their spectral energy distributions. Therefore...

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Bibliographic Details
Main Authors: Su, Kate Y. L., De Buizer, James M., Rieke, George H., Krivov, Alexander V., Löhne, Torsten, Marengo, Massimo, Stapelfeldt, Karl R., Ballering, Nicholas P., Vacca, William D.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
circumstellar matter
infrared: stars
planetary systems
stars: individual (is an element of Eri)
Online Access:http://hdl.handle.net/10150/624715
http://arizona.openrepository.com/arizona/handle/10150/624715

Internet

http://hdl.handle.net/10150/624715
http://arizona.openrepository.com/arizona/handle/10150/624715

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