Journal article icon

Journal article

Dynamical models to explain observations with SPHERE in planetary systems with double debris belts

Abstract:

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...

Expand abstract
Publication status:
Published
Peer review status:
Peer reviewed

Actions


Access Document


Authors


More from this funder
Name:
Seventh Framework Programme
Grant:
312430
More from this funder
Name:
Sixth Framework Programme
Grant:
RII3-Ct-2004-001566
More from this funder
Name:
Netherlands Research School for Astronomy
More from this funder
Name:
Max Planck Institute for Astronomy
More from this funder
Name:
Italian National Institute for Astrophysics
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:
1432-0746
ISSN:
0004-6361
Language:
English
Keywords:
Pubs id:
pubs:734860
UUID:
uuid:e96f1bf5-3629-41fa-a71d-aa08bead67fa
Local pid:
pubs:734860
Source identifiers:
734860
Deposit date:
2018-02-05

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP