Clusters of galaxies at the Planck time

Details Clusters of galaxies at the Planck time Clusters of galaxies at the Planck time

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sf2a.conf...13p&link_type=abstract

SF2A-2009: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, held 29 June - 4 July 2009 in

Astronomy and Astrophysics

Astrophysics

Scientific paper

Nodes of the filaments forming the cosmic web traced by the dark and
baryonic matter, galaxy clusters are the place of many physical
processes that shape a complex interaction between the formation and
the evolution of galaxies, their environment and large scale
structures. Their various components can be observed from X-ray to
radio wavelengths. The ESA space mission Planck surveyor, lauched on
May 14^{th} this year, is currently surveying the whole sky from
sub-millimeter to centimeter wavelengths. Hundreds of new clusters
are expected to be detected from the this survey. I review here
various axis of research in the field of galaxy clusters studies,
and I investigate the prospect of the detection of new distant
clusters with the Planck satellite, which is expected to shed new
light in the field of the formation and evoltution of large scale
structures, and to provide cosmological constraints complementary to
those derived from the CMB measurements.

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