What Sets the Radial Locations of Warm Debris Disks?
The architectures of debris disks encode the history of planet formation in these systems. Studies of debris disks via their spectral energy distributions (SEDs) have found infrared excesses arising from cold dust, warm dust, or a combination of the two. The cold outer belts of many systems have bee...
| Main Authors: | , , , |
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| Other Authors: | |
| Language: | en |
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IOP PUBLISHING LTD
2017
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| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/625773 http://arizona.openrepository.com/arizona/handle/10150/625773 |