Méthodes directes Galaxy evolution Lithosphérique Collisional relaxation Configuration interaction ALPS Techniques radial velocities Planets and satellites formation Tomography Données multicomposantes Stars late-type Asteroid Solar wind Density 67P/Churyumov-Gerasimenko Planets and satellites dynamical evolution and stability Asteroids general Local optimization Parallel computation Accretion Seismic imaging Methods observational Achernar Accretion disks 3D Tomographie multiparamètres ASTEROIDS INDIVIDUAL 6 HEBE Planet-disk interactions Taylor-Green Densité Amortissement Landau Acceleration of particles Stars fundamental parameters Approximations de rang-faible Astrophysics - Earth and Planetary Astrophysics Galaxy abundances Methods data analysis Methods statistical Radiative transfer Inversion de formes d'ondes Surveys Télésismique Computational seismology Simulation Inverse theory Astrophysics - Solar and Stellar Astrophysics Imagerie sismique Dipole moment surface Non-linear inverse problem Tomographie Alps Methods numerical Waveform inversion Theory ADMM Stars activity Protoplanetary disks Problème inverse non-linéaire Compound regularization Supernovae general Methane Frequency-domain analysis Ab initio intensities Théorie Stars atmospheres Plasmas Seismic waves Alpes Imagerie sismique quantitative haute résolution Systèmes linéaires creux Seismic anisotropy Magnetohydrodynamics Hydrodynamics Gravitation Wave propagation Instabilities ASTEROIDE Circumstellar environment Techniques photometric ArfGAP1 Galaxy disk Adjoint state method Turbulence Controlled source seismology Geophysical techniques Multifrontal method Molecular dynamics Dynamo Stars abundances Long-range interacting systems Planetary systems Planets and satellites detection Algèbre linéaire Minor planets Lithospheric Teleseismic Optimisation locale Frequency domain Full-waveform inversion Amphipathic helix