index - Laboratoire d' Astrophysique de Marseille

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

 

 

 

 

Nos dépôts

3 136

Nos notices

3 216

Nos thématiques

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

 

 

 

Nos collaborations internationales