Rich galaxy clusters as microwave sources - Predicted count curves

Details Rich galaxy clusters as microwave sources - Predicted count curves Rich galaxy clusters as microwave sources - Predicted count curves

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..339k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, May 1986, p. 339-352) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

1

Extragalactic Radio Sources, Galactic Clusters, Microwave Spectra, Red Shift, Background Radiation, Cosmology, Galactic Evolution, Intergalactic Media, Luminosity

Scientific paper

The properties which make galaxy clusters objects of interest in observational cosmology are discussed. It is noted that clusters may be invaluable objects for applying the classic cosmological tests: source counts and the angular size-redshift relation. Data are presented which show that in the microwave range, radio-source counts may be dominated by distant clusters of galaxies. The predicted log N and log S curves deviate significantly from counts at centimeter and decimeter wavelengths.

Affiliated with

Also associated with

No associations

Rating

Rich galaxy clusters as microwave sources - Predicted count curves does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Rich galaxy clusters as microwave sources - Predicted count curves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rich galaxy clusters as microwave sources - Predicted count curves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1833986