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MAPP : project team

Par Jean-Francois Donati - 20/05/2008

 

MAPP:
project team


© C Liljegren & D Dravins, Lund

The MAPP core team spreads between LATT (Toulouse), ENS (Lyon & Paris), LAOG (Grenoble), IAP (Paris) and CEA (Saclay). The full list is given below. Collaborators from Europe, North-America and Asia are also expected to participate in the project.

MAPP is funded by the French "Agence Nationale de la Recherche" (ANR); in particuliar, two 2-yr postdoctoral fellowships are granted to this project and will soon be advertised on this page. MAPP is also supported by the French national CNRS program on Stellar Physics (PNPS).
Team Persons Implication (FTE)Role & expertise
LATT/UMR 5572 (Toulouse)Donati80% project coordinator - definition and setup of the observing program - data reduction and analysis - tomographic modeling of magnetic topologies of protostars and accretion discs - organizing regular meetings between team members and external experts
new postdoc100% tomographic modeling of magnetic topologies of protostars and accretion discs
Rincon10% theoretical disc dynamos - 3D MHD numerical simulations
ENS/UMR 5574 (Lyon)Chabrier60% 3D MHD collapse of magnetised molecular clouds - interaction between magnetic field and convection - implementation of physical ingredients in numerical models (opacity, radiative transfer, equation of state) - modelling of accretion processes
Mulet-Marquis100% collapse of magnetised molecular clouds
Baraffe20% state-of-the-art theoretical models of very low-mass stars - stellar evolution models
ENS/UMR 8112 (Paris)Hennebelle20% collapse of magnetised molecular clouds - 3D MHD numerical simulations with AMR
LAOG/UMR 5571 (Grenoble)Bouvier30% observations of magnetic field strength and topology at the surface of young stars and in their inner disks - characterizing and modelling the magnetic star-disk interaction and the angular momentum evolution of young stars
Dougados30% observations and modeling of magnetized mass-loss in protostars and protostellar accretions discs - observations of magnetic topologies at the surfaces of classical T Tauri stars
Ferreira20% numerical simulations of magnetised mass-loss from protostellar accretion discs - numerical simulations of magnetospheric accretion between protostars and their accretion discs
Zanni10% numerical simulations of magnetospheric accretion between protostars and their accretion discs
Ménard10% observations of protostellar accretion discs at larger radii
IAP/UMR 7095Terquem30% MHD simulations of magnetic accretions discs - planet migration in magnetic accretion discs
CEA/UMR 7158Fromang10% MHD simulations of magnetic accretions discs - planet migration in magnetic accretion discs

 

 

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