A COMPREHENSIVE DUST MODEL APPLIED TO THE RESOLVED BETA PICTORIS DEBRIS DISK FROM OPTICAL TO RADIO WAVELENGTHS
We investigate whether varying the dust composition (described by the optical constants) can solve a persistent problem in debris disk modeling-the inability to fit the thermal emission without overpredicting the scattered light. We model five images of the beta Pictoris disk: two in scattered light...
Main Authors: | , , , |
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Other Authors: | |
Language: | en |
Published: |
IOP PUBLISHING LTD
2016
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Online Access: | http://hdl.handle.net/10150/621242 http://arizona.openrepository.com/arizona/handle/10150/621242 |