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
Nos dépôts
2 747
Nos notices
3 276
Nos thématiques
Galaxies statistics
Galaxies kinematics and dynamics
Stars fundamental parameters
Galaxies
Spectroscopy
Minor planets
Ultraviolet galaxies
Cosmology
Galaxies ISM
Instrumentation adaptive optics
Exoplanets
Quasars absorption lines
Data analysis
Planetary systems
Galaxies stellar content
Quasars general
Adaptive optics
Techniques photometric
Dark matter
Galaxies photometry
Dark energy
Galaxies luminosity function
Galaxies Evolution
Planets and satellites fundamental parameters
Catalogs
Gravitational lensing strong
Telescopes
Cosmology observations
Methods numerical
Stars formation
Galaxies distances and redshifts
Galaxies clusters general
Neutrino detector
Galaxies general
ISM clouds
Planets and satellites detection
Galaxy formation
OPTIQUE ADAPTATIVE
Galaxies interactions
Dust
Radiative transfer
Galaxies spiral
Techniques polarimetric
Galaxies starburst
Galaxies active
High-redshift galaxies
Astrophysics - Astrophysics of Galaxies
Surveys
Methods statistical
Astrophysics - Earth and Planetary Astrophysics
Galaxies fundamental parameters
H II regions
Planets and satellites atmospheres
Astrophysics
Adaptive Optics
Comets general
ISM molecules
Methods observational
Protoplanetary disks
Cosmological parameters
Galaxy evolution
Cosmic background radiation
Astrophysics - Solar and Stellar Astrophysics
Galaxies star formation
ANTARES
Gravitational lensing weak
Galaxies structure
Supernovae general
Large-scale structure of Universe
67P/Churyumov-Gerasimenko
Techniques spectroscopic
Techniques high angular resolution
X-rays galaxies clusters
CD
Galaxies evolution
Photometry
Galaxies clusters individual Virgo
Techniques radial velocities
Infrared galaxies
Mass function
Techniques image processing
Comets
Galaxies groups general
Astrophysics - Cosmology and Nongalactic Astrophysics
Submillimeter galaxies
Galaxies dwarf
Infrared ISM
Intergalactic medium
Submillimeter ISM
Galaxies abundances
Instrumentation high angular resolution
Gravitational lensing
Galaxies high-redshift
Methods data analysis
Extinction
Planets and satellites composition
Galaxies formation
Galaxies haloes
Astrophysics - Instrumentation and Methods for Astrophysics
Star formation
Nous suivre !
Nos collaborations internationales