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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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J. Cabrera, Sz. Csizmadia, G. Montagnier, M. Fridlund, M. Ammler-von Eiff, et al.. Transiting exoplanets from the CoRoT space mission. XXVII. CoRoT-28b, a planet orbiting an evolved star, and CoRoT-29b, a planet showing an asymmetric transit. Astronomy & Astrophysics - A&A, 2015, 579, pp.id.A36. ⟨10.1051/0004-6361/201424501⟩. ⟨hal-01170412⟩
Nos dépôts
3 210
Nos notices
3 221
Nos thématiques
Infrared ISM
Galaxies starburst
Gravitational lensing strong
Stars formation
Techniques polarimetric
Large-scale structure of Universe
Galaxy formation
Galaxies haloes
Galaxies formation
Mass function
Adaptive optics
Planets and satellites fundamental parameters
Exoplanets
ISM molecules
Stars fundamental parameters
Planetary systems
Galaxies interactions
Planets and satellites composition
Cosmology
Dark matter
Comets general
Spectroscopy
Galaxies active
Galaxies clusters individual Virgo
Planets and satellites atmospheres
Instrumentation adaptive optics
Quasars general
Galaxies groups general
Galaxies kinematics and dynamics
Galaxies abundances
Gravitational lensing weak
Techniques high angular resolution
Astrophysics - Astrophysics of Galaxies
Methods statistical
ANTARES
Techniques spectroscopic
Photometry
Galaxies luminosity function
Galaxies photometry
Instrumentation high angular resolution
Protoplanetary disks
Astrophysics - Earth and Planetary Astrophysics
Planets and satellites detection
Cosmic background radiation
Techniques radial velocities
Telescopes
Galaxies high-redshift
Galaxies structure
X-rays galaxies clusters
Dust
Supernovae general
Galaxies fundamental parameters
Star formation
Submillimeter ISM
Submillimeter galaxies
Surveys
Galaxies statistics
Ultraviolet galaxies
Astrophysics
Astrophysics - Cosmology and Nongalactic Astrophysics
OPTIQUE ADAPTATIVE
Data analysis
Neutrino detector
Galaxies evolution
Methods observational
Extinction
High-redshift galaxies
Techniques image processing
Catalogs
Cosmology observations
Planets and satellites gaseous planets
Dark energy
H II regions
Methods data analysis
Techniques photometric
Intergalactic medium
Galaxies ISM
Galaxies clusters general
Adaptive Optics
Galaxies
Galaxies stellar content
Galaxies general
67P/Churyumov-Gerasimenko
Comets
Galaxy evolution
Methods numerical
Quasars absorption lines
Galaxies distances and redshifts
Cosmological parameters
Galaxies Evolution
Galaxies dwarf
Infrared galaxies
Astrophysics - Solar and Stellar Astrophysics
Radiative transfer
ISM clouds
Gravitational lensing
Galaxies spiral
Minor planets
Astrophysics - Instrumentation and Methods for Astrophysics
Galaxies star formation
Nous suivre !
Nos collaborations internationales
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