Journal article
Dynamical models to explain observations with SPHERE in planetary systems with double debris belts
- Abstract:
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Context
A large number of systems harboring a debris disk show evidence for a double belt architecture. One hypothesis for explaining the gap between the debris belts in these disks is the presence of one or more planets dynamically carving it. For this reason these disks represent prime targets for searching planets using direct imaging instruments, like the Spectro-Polarimetric High-constrast Exoplanet Research (SPHERE) at the Very Large Telescope.
Aims
The goal...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Version of record, pdf, 3.9MB, Terms of use)
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- Publisher copy:
- 10.1051/0004-6361/201731426
Authors
- Publisher:
- EDP Sciences
- Journal:
- Astronomy & Astrophysics More from this journal
- Volume:
- 611
- Pages:
- A43
- Publication date:
- 2018-03-28
- Acceptance date:
- 2017-10-06
- DOI:
- EISSN:
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1432-0746
- ISSN:
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0004-6361
- Language:
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English
- Keywords:
- Pubs id:
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pubs:734860
- UUID:
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uuid:e96f1bf5-3629-41fa-a71d-aa08bead67fa
- Local pid:
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pubs:734860
- Source identifiers:
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734860
- Deposit date:
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2018-02-05
Terms of use
- Copyright holder:
- European Southern Observatory
- Copyright date:
- 2018
- Notes:
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Reproduced with permission from Astronomy and Astrophysics, © ESO 2018.
This is the published version of the article. This version is also available online from EDP Sciences at: http://dx.doi.org/10.1051/0004-6361/201731426
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