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Dynamical models to explain observations with SPHERE in planetary systems with double debris belts
Research output
:
Contribution to journal
›
Article
›
peer-review
Department of Astronomy, Geodesy, Ecology and Environmental Monitoring
Institute of Natural Sciences and Mathematics
Overview
Cite this
DOI
https://doi.org/10.1051/0004-6361/201731426
Final published version
T. Kopytova
And 49 others
C. Lazzoni
S. Desidera
F. Marzari
A. Boccaletti
M. Langlois
D. Mesa
R. Gratton
Q. Kral
N. Pawellek
J. Olofsson
M. Bonnefoy
G. Chauvin
A. M. Lagrange
A. Vigan
E. Sissa
J. Antichi
H. Avenhaus
A. Baruffolo
J. L. Baudino
A. Bazzon
J. L. Beuzit
B. Biller
M. Bonavita
W. Brandner
P. Bruno
E. Buenzli
F. Cantalloube
E. Cascone
A. Cheetham
R. U. Claudi
M. Cudel
S. Daemgen
V. De Caprio
P. Delorme
D. Fantinel
G. Farisato
M. Feldt
R. Galicher
C. Ginski
J. Girard
E. Giro
M. Janson
J. Hagelberg
T. Henning
S. Incorvaia
M. Kasper
H. Lecoroller
L. Lessio
R. Ligi
Original language
English
Article number
A43
Number of pages
22
Journal
Astronomy and Astrophysics
Volume
611
DOIs
https://doi.org/10.1051/0004-6361/201731426
Publication status
Published -
28 Mar 2018
WoS ResearchAreas Categories
Astronomy & Astrophysics
ASJC Scopus subject areas
Astronomy and Astrophysics
Space and Planetary Science
Research areas
Instrumentation: high angular resolution, Kuiper belt: general, Methods: analytical, Methods: observational, Planet-disk interactions, Techniques: image processing, methods: observational, KUIPER-BELT, PARTICLES, GIANT PLANETS, CHAOTIC ZONE, DISCOVERY, DUST, EVOLUTION, techniques: image processing, ECCENTRICITY, methods: analytical, instrumentation: high angular resolution, planet-disk interactions, DISK, HR 8799
ID: 7034986