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

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. BazzonJ. 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, T. Kopytova, H. Lecoroller, L. Lessio, R. Ligi, A. L. Maire, F. Ménard, M. Meyer, J. Milli, D. Mouillet, S. Peretti, C. Perrot, D. Rouan, M. Samland, B. Salasnich, G. Salter, T. Schmidt, S. Scuderi, E. Sezestre, M. Turatto, S. Udry, F. Wildi, A. Zurlo

*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

Fingerprint

Dive into the research topics of 'Dynamical models to explain observations with SPHERE in planetary systems with double debris belts'. Together they form a unique fingerprint.

Physics