Loading...
Le LAM constitue l’un des plus importants instituts de recherche publique en France dans le domaine de l’Astrophysique et associe la recherche fondamentale et le développement d’instrumentation pour les grands télescopes au sol et dans l’espace. Il fait partie de l'Institut OSU Pythéas. Le LAM est une Unité Mixte de Recherche (n°7326) avec comme tutelles le CNRS-INSU, l’Université Aix-Marseille (AMU) et le CNES.
Nos derniers dépôts
![Chargement de la page](/img/loading.gif)
Nos dépôts
2 859
Nos notices
![Chargement de la page](/img/loading.gif)
Nos thématiques
Methods observational
Gravitational lensing strong
Galaxies clusters individual Virgo
Galaxies structure
Adaptive optics
Astrophysics - Instrumentation and Methods for Astrophysics
Comets
Surveys
Extinction
ISM clouds
Spectroscopy
Galaxies stellar content
Planets and satellites detection
Planets and satellites fundamental parameters
Stars fundamental parameters
Galaxies abundances
Infrared galaxies
Gravitational lensing
Astrophysics - Earth and Planetary Astrophysics
Galaxies active
Astrophysics - Astrophysics of Galaxies
Galaxies star formation
Instrumentation adaptive optics
Galaxies ISM
Gravitational lensing weak
Infrared ISM
Protoplanetary disks
Techniques spectroscopic
Quasars general
Techniques photometric
Galaxies interactions
Instrumentation high angular resolution
Planetary systems
Galaxies kinematics and dynamics
Astrophysics - Cosmology and Nongalactic Astrophysics
Galaxies photometry
Galaxies
Galaxies clusters general
OPTIQUE ADAPTATIVE
ISM molecules
Radiative transfer
Cosmology
Data analysis
Galaxies haloes
CD
Cosmology observations
Galaxies fundamental parameters
Ultraviolet galaxies
Mass function
Comets general
Telescopes
Submillimeter ISM
H II regions
X-rays galaxies clusters
Galaxy formation
ANTARES
Galaxies evolution
Neutrino detector
Star formation
Photometry
Dust
Techniques image processing
Galaxies luminosity function
67P/Churyumov-Gerasimenko
Methods statistical
Dark matter
Galaxies dwarf
Cosmic background radiation
Exoplanets
Galaxy evolution
Techniques high angular resolution
Catalogs
Galaxies spiral
Quasars absorption lines
Astrophysics
Planets and satellites composition
Submillimeter galaxies
Methods data analysis
Galaxies statistics
Supernovae general
Galaxies starburst
Large-scale structure of Universe
Galaxies distances and redshifts
Galaxies formation
Intergalactic medium
Methods numerical
Dark energy
Galaxies high-redshift
High-redshift galaxies
Adaptive Optics
Galaxies groups general
Astrophysics - Solar and Stellar Astrophysics
Minor planets
Techniques polarimetric
Galaxies Evolution
Galaxies general
Stars formation
Planets and satellites atmospheres
Cosmological parameters
Techniques radial velocities
Nous suivre !
Nos collaborations internationales