Cosmology with multiwavelength observations of clusters of galaxies

Details Cosmology with multiwavelength observations of clusters of galaxies Cosmology with multiwavelength observations of clusters of galaxies

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..554k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 10, p. 554 - 561 (2003)

Mathematics

Logic

Cosmology, Clusters Of Galaxies, Multiwavelength Observations

Scientific paper

As the largest structure in the Universe, clusters of galaxies have widely been used as a probe of cosmological parameters and density fluctuations. The advent of new observatories such as Chandra, XMM-Newton and WMAP is now leading us to a new era of researches of galaxy clusters. We outline the significance of cosmological studies with multiband observations of galaxy clusters, including that of the Sunyaev-Zel'dovich effect, and discuss their future directions.

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