LERMA UMR8112

Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique et Atmosphères



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Galaxies and Cosmology

by Françoise Combes - published on , updated on

This pole has several themes of research, which can be gathered in:

  1. The early universe: inflation, cosmic backgrounds, reionization
  2. Dark matter: Cold, warm or modified gravity?
  3. Galaxy formation: high-z early galaxies, secular evolution and mergers
  4. Black holes and galaxies: AGN, starbursts, symbiotic growth and feedback
  5. Star formation efficiency, history and stellar populations

See Activities of the group for more details

The pole Galaxies and Cosmology includes a group working on the cosmic microwave background (CMB), who has a major role in the Planck mission, another group working on the standard model of the Universe, the inflation theory compared to observations. Another team studies through numerical simulations the epoch of reionization of the Universe (EoR, cf Fig 1), and in particular the preparation of SKA (Embrace prototype, key projects on pathfinders, etc..). Pioneering work has been done on cooling flows and the presence of cold molecular gas near the brightest cluster galaxies. The nature of dark matter, and investigation on alternative theories of modified gravity have been probed through galaxy dynamics and observations. A thorough study of AGN fueling and feedback has been carried out, addressing black hole growth history and galaxy evolution.

Figure 1: Simulations of the HI-21cm emission during the Reionization Epoch (EoR). Example of cross sections of the 21-cm light cones: dTb from raw simulation data (left) , dTb with SKA-like noise et resolution (middle) and dTb with LOFAR-like noise and resolution (right). False colors show the differential brightness temperature Tb in mK.

Another team works both on the observation of local galaxies, the physics of galaxies in clusters, galaxies at high redshift (cf Fig 2), and on the dynamical theories for the evolution and formation of galaxies, on large-scale star formation and the cosmic star formation history.
Multi-wavelengths observations are used extensively, in the millimeter and centimeter with the instruments of IRAM, the VLA and now ALMA since 2011-12, infrared and far-infrared with the satellites Spitzer and Herschel, optical and near-infrared with the CFHT and ESO. Team members are leaders in key programs, such as the NUGA consortium on the IRAM interferometer, the consortium PrimGal on the VLT, or major programs at IRAM (which will be completed by NOEMA in the near future) on distant galaxies, and the observation of galaxies at large z with APEX, Plateau de Bure and ALMA, which data are now frequently arriving to the various groups. One group is actively preparing for the SKA.

Figure 2: One of the objects of the sample in the Large Program PHIBSS at IRAM PdB at z=1.2 Left: Superposition of the CO map (in red, obtained with the interferometer of IRAM), with the images in band I (in green) and band V (in blue) obtained with the Hubble Space telescope. The CO(3-2) line, redshifted to 2mm, was observed with an angular resolution of 0.6" x0.7" (beam indicated by the grey hatched ellipse). Right: Velocity field of the galaxy: blue indicates negative velocity (approaching side), and red positive velocity (recessing side).

One specialty of the pole is also heavy numerical simulations, and the team competed at a very high level in the HORIZON project program of formation of galaxies in a cosmological context. Always larger and more impressive simulations are now going on with the supercomputers at GENCI (Curie at CEA, IDRIS, CINES), and locally use of the meso-center and local momentum cluster is favoring the exploitation and post-processing.

Figure 3 : The barred spiral galaxy NGC 1433, observed with ALMA in CO(3-2). The central black hole is an active nucleus (AGN) which expels some molecular gas, quenching the star formation.

View online : Activities of the group

Séminaires à venir

Vendredi 17 avril 2020, 14h00
Salle de l'atelier, Paris
Patricia TISSERA
Universidad Andres Bello, Santiago, Chili
 
Vendredi 24 avril 2020, 14h00
Salle de l'atelier, Paris
Tba
Philippe ANDRE
CEA
 
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