Name: Phase Transitions in Astrophysics, from ISM to Planets
Start: 2017-05-07T09:00:00+02:00
End: 2017-06-02T18:00:00+02:00
Location: Nordita, Stockholm

50 years of thermal instability : what have we learned ? what are the new questions ?

Characterisation of Exoplanets, how to understand their mass, radius, and atmospheric composition

Clustering and dynamic decoupling of dust grains in turbulent molecular clouds

Convection on Jupiter's icy moons as a consequence of tidal forces

Critical phenomena, nonlinear dynamics and the formation and detection of planets

Detection and characterization of planets around M Dwarfs

Discussion on NASA Europa mission

Disentangling the structures in debris disks: Planets or just gas?

Effect of Phase Transitions on Turbulent Transport

Effects of the multi-phase character of the interstellar medium on the Galactic dynamo

Feedback and interactions from low-mass stars in the Coronet cluster

Formation and evolution of filaments in the interstellar medium

Fragmentation of a Filamentary Molecular Cloud Permeated by Perpendicular Magnetic Field

Geophysical test for habitability in icy ocean worlds

Implementing a Radially Efficient Poisson Equation Solver to Investigate Tidal Downsizing

Jupiter internal structure and the first Juno results

On the different kinds of superfluid vortices in the interior of neutron stars

Phase Transition Dynamics of ISM: The Formation of Molecular Clouds and Galactic Star Formation

Practical Python for Researchers (1st part)

Practical Python for Researchers (2nd part)

Practical Python for Researchers (3rd part): discussion

Presentation of an all-Mach regime solver

Python installation tutorial

Reduced gas accretion onto Super-Earths and ice giants

Riddles from the AU Microscopii system

Shining Light on the Dark ISM

Smooth Particle MHD, method, expectatives and strategies

Solving radiation and hydrodynamics using a moments model

Some aspects of protoplanetary disc formation and evolution

The Dark Milky Way: Probing our Galaxy’s Hidden Gas

The HI turbulence: temperature distribution, buildup of molecular clouds, and ineffective stellar feedback

The Magnetized and multiphase ISM as seen by Planck

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Phase Transitions in Astrophysics, from ISM to Planets