Program of the meeting

• Adressed topics: formation and stability of vortices, self-gravitating structures, dust-laden vortices, possible observations in protoplanetary disks .

Please, notes that the meeting will take place on two different sites !

List of the contributions

• Aubert Oriane : (T) Vortices in rotating and stratified flows: aspect ratio and sustainability

• Barranco Joseph : (T) A new approach for strong dust-gas coupling in protoplanetary disks (canceled)

• Birnstiel Tilman : (T) Transition Disks - Grain Growth, Planets, or Photoevaporation ?

• Boehler Yann: (T) Dust settling with ALMA: Simulations and predictions

• Crespe Elisabeth: (T) The RWI in 2D viscous Protoplanetary disks (canceled)

• Dullemond Cornelis: (R) Observational appearance of protoplanetary disks: a review talk

• Faure Julien: (T) Dynamics of the inner edge of the dead zone

• Fromang Sebastien : (T) Meridional circulation in turbulent protoplanetary disks

• Hendrix Tom : (T) Dust dynamics of astrophysical fluids

• Hubbard Alexander : (T) The short circuit instability in protoplanetary disk MRI turbulence

• Johansen Anders : (R) Streaming instabilities and planetesimal formation (canceled)

• Jung Manuel: (P1) Planet-disk interaction revisited

• Klahr Hubert: (T) Disk Weather: Baroclinic Instability and Vortex Amplification - From physical conditions in disks to 3D global radiation hydro simulations

• Lambrecht Michiel : (T) Rapid growth of gas-giant cores by peeble accretion

• Latter Henrik : (T) The resistive double-diffusive instability in protoplanetary disks

• Lesur Geoffroy : (R) The baroclinic instability in local accretion disc models: mechanism and secondary instabilities

• Li Hui: (T) Planet Migration in 3-D Self-Gravitating Disks

• Lin Min-Kai: (T) Vortices and spirals at gap edges in 3D self-gravitating disc-planet simulations

• Lovelace Richard: (R) Global 3D MHD Simulations of Waves in Accretion Discs

• Lyra Wladimir: (R) Elliptic and magneto-elliptic instabilities

• Mamatsashvili George: (R) Dynamics of perturbation modes in self-gravitating magnetized disks: new effect of Keplerian differential rotation

• Marcus Philipp: (T) Self-Replication of Vortices and Critical Layers in Keplerian Disks

• Meheut Heloise : (T) Rossby vortices in the context of planetesimal formation

• Meheut Heloise : (T) Dust-trapping Rossby vortices in Protoplanetary disks'

• Meru Farzana: (T) Triggered fragmentation in gravitationally unstable discs: forming fragments at small radii

• Oishi Jeffrey : (R) The Heavy-Core Instability in Dust Gathering PP Vortices

• Paardekooper Sijme-Jan : (R) Vortex migration in Protoplanetary disks

• Papaloizou John : (R) Instabilities of axisymmetric structures and vortices in protoplanetary disks

• Pessah Martin : (T) On Angular Momentum Transport in PP disk boundary layers around young stars

• Railton Anna : (T) On the stability of dust laden vortices

• Regaly Zolt : (T) Possible planet forming regions in submillimeter images

• Richard Samuel : (T) The structure and evolution of 3D Rossby vortices

• Richard Samuel : (T) 2D and 3D simulations of the baroclinic instability

• Ros Katrin : (T) Ice condensation as a planet formation mechanism

• Ruge Jean-Phjlip : (T) Tracing planets in protoplanetary disks

• Snytnikov Valeriy : (T) Initial stages of circumstellar disc formation and following evolution. Physical model

• Snytnikov Valeriy : (T) What gravitational instabilities we need to form collapsing clumps in PP disks

• Stoyanovskaya Olga : (T) Numerical modeling of gravitational instability outcomes in multiphase PP discs

• Surville Clement : (T) Structure and migration of 2D vortices

• Umurhan Orkan : (T) The unsteady competition between Rossby and strato-rotational instabilities in PP disks

• Watanabe Keisuke : (P2) Linear analysis of thermal instability: A possible dust accumulation process

• Zakhozhay Olga : (T) Spectral energy distributions of fragmenting protostellar disks

• Outline

• (P): poster presentation

• (T): standard talk – 15mn + 5 mn

• (R): review talk – 30 mn + 10 mn