Far-Infrared Emission of Intracluster Dust (ICD)

Details Far-Infrared Emission of Intracluster Dust (ICD) Far-Infrared Emission of Intracluster Dust (ICD)

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000isass..14..107a&link_type=abstract

The Institute of Space and Astronautical Science Report SP No. 14, p. 103-114.

Astronomy and Astrophysics

Astronomy

Galaxies, Elliptical, Evolution, Cluster, Dust, Infrared

Scientific paper

In the young universe, clusters of galaxies could be bright FIR-Submm sources due to the dust emissions from young ellipticals. The intracluster dust (ICD) could also contribute to the FIR-Submm emissions considerably, but the ICD is fragile in the ambient hot ICM. Therefore, a chance to detect the ICD emission would be much smaller than the dust emissions from galaxies. Dust emissions from elliptical galaxies (EROs) in the young Coma cluster at a distance of z=2-3 would be easily detected by a future mission of H2L2 satellite, thus the FIR-Submm survey would become a powerful tool for searching high-z clusters.

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