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| Stars I |
Star counts, radial velocities, proper motions,
metallicities and ages |
Annie Robin (France) |
| Stars II |
Large-scale non-equilibrium structures |
Vasily Belokurov (UK) |
| Stars III |
Non-equilibrium dynamics and radial migration in the disc |
Alice Quillen (USA) |
| Populations |
Star-formation histories, metallicity distributions and
luminosity functions of disk, bulge & halo |
Rosie Wyse (USA) |
| ISM I |
Measures of ISM density (absorption, emission at various
frequencies, polarization, Faraday rotation, dust to gas ratio) |
?? |
| ISM II |
Gas dynamics: motions driven by bar and spiral structure;
impact on large-scale gas distribution (x2 ring, molecular ring or
arms?); validity of kinematical distances |
Lia Athanassoula (France) |
| Mass distribution |
Exploiting horizontal and vertical dynamics of disc,
dynamics of halo structures and satellites |
Amina Helmi (Netherlands) |
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Methods
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| Schwarzschild |
Introduction to orbit-superposition models. How do we fit
such a model to a catalogue? |
Roeland van der Marel (USA) |
| Tori |
Torus modelling as an extension of Schwarzschild; respects
in which it supercedes Schwarzschild |
James Binney (UK) |
| N-body |
In what detail can we represent the MW in a conventional
N-body model? |
Victor Debattista (UK) |
| M2M |
To what extent does M2M overcome limitations of conventional
N-body? |
Ortwin Gerhard (Germany) |
| Projection |
Projecting models into the observational domain; can we
develop common tools for this? what would be the standard interfaces? |
Herwig Dejonge (Belgium) |
| Dust-fitting |
Given the Gaia catalogue, an NIR catalogue (VHS?) and a
dynamical model, how to build a dust model? |
Jacques Lepine (Brazil) |
| Fitting |
How to optimise complex models? Will the computational scale
be worryingly large? |
Prasenjit Saha (Switzerland) |
| Summary |
|
Ken Freeman (Australia) |
Contacts:
E-mail: binney@thphys.ox.ac.uk
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