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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
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Sharon E. Meidt, Adam K. Leroy, Miguel Querejeta, Eva Schinnerer, Jiayi Sun, et al.. The Organization of Cloud-scale Gas Density Structure: High-resolution CO versus 3.6 μm Brightness Contrasts in Nearby Galaxies. The Astrophysical Journal, 2021, 913, 16 pp. ⟨10.3847/1538-4357/abf35b⟩. ⟨hal-03585905⟩
Nos dépôts
2 701
Nos notices
3 295
Nos thématiques
Methods statistical
Galaxies general
Dark energy
Quasars absorption lines
Photometry
Cosmic background radiation
Telescopes
Methods data analysis
Galaxies spiral
Neutrino detector
Catalogs
Galaxies distances and redshifts
Galaxies groups general
Ultraviolet galaxies
Submillimeter ISM
Dark matter
Cosmology observations
Galaxy formation
Astrophysics - Earth and Planetary Astrophysics
Instrumentation high angular resolution
Dust
X-rays galaxies clusters
Techniques polarimetric
Spectroscopy
Planets and satellites atmospheres
Astrophysics - Instrumentation and Methods for Astrophysics
Stars fundamental parameters
Gravitational lensing
Infrared galaxies
Galaxies haloes
High-redshift galaxies
Techniques high angular resolution
Galaxies stellar content
Large-scale structure of Universe
Submillimeter galaxies
Galaxies kinematics and dynamics
CD
Planetary systems
67P/Churyumov-Gerasimenko
Star formation
Gravitational lensing weak
Galaxies active
Galaxies
Adaptive Optics
Galaxies clusters general
Stars formation
Astrophysics - Solar and Stellar Astrophysics
Galaxies structure
Supernovae general
ISM clouds
Galaxies luminosity function
Cosmological parameters
Galaxies Evolution
Galaxies ISM
Galaxies fundamental parameters
OPTIQUE ADAPTATIVE
Astrophysics - Astrophysics of Galaxies
Galaxies abundances
Quasars general
Planets and satellites composition
Extinction
Astrophysics
Galaxies statistics
Galaxy evolution
Galaxies formation
Surveys
Galaxies star formation
H II regions
Galaxies high-redshift
Infrared ISM
ANTARES
Galaxies photometry
Galaxies interactions
Techniques image processing
Comets general
Techniques radial velocities
Data analysis
Techniques spectroscopic
Methods observational
Galaxies starburst
Galaxies dwarf
Galaxies clusters individual Virgo
Planets and satellites detection
Galaxies evolution
Individual
ISM molecules
Mass function
Adaptive optics
Comets
Exoplanets
Methods numerical
Cosmology
Gravitational lensing strong
Astrophysics - Cosmology and Nongalactic Astrophysics
Instrumentation adaptive optics
Radiative transfer
Protoplanetary disks
Planets and satellites fundamental parameters
Intergalactic medium
Techniques photometric
Nous suivre !
Nos collaborations internationales