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Program

Program of the meeting


"Fusion of Rossby vortices" "A baroclinic vortex"




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

The preliminary program is under construction.

Monday 17th

Tuesday 18th

Wednesday 19th

Thursday 20th

9:00-10:30

10:30-11:00

break

break

break

11:00-12:15

12:30-14:00

welcome

lunch

Lunch

lunch

14:00-15:30

Boat tour
Free afternoon

15:30-16:00

break

break

16:00-18:00

End

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

  • 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

  • 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

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

  • 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: (T) Triggering the RWI in a realistic dead zone environment (TBC)

  • Lyra Wladimir: (T) Magneto elliptical instability(title TBC)

  • 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

  • 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) A review on disk instabilities (title TBC)

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

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

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

  • Richard Samuel: (T) 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) Various families of vortices and their migration

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

  • Zakhozhay Olga: (T) New method of age determination for substars with PP disks


  • Outline

  • (P): poster presentation

  • (T): standard talk – 15mn + 5 mn

  • (R): review talk – 30 mn + 10 mn