Hubble constant from X-ray and microwave observations of clusters of galaxies

Details Hubble constant from X-ray and microwave observations of clusters of galaxies Hubble constant from X-ray and microwave observations of clusters of galaxies

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cosp.meetr....c&link_type=abstract

COSPAR, Plenary Meeting, 21st, Innsbruck, Austria, May 29-June 10, 1978, Paper. 13 p. Research supported by the Consiglio Nazion

Statistics

Applications

Astrometry, Galactic Clusters, Hubble Diagram, X Ray Sources, Applications Of Mathematics, Bremsstrahlung, Cosmology, Distance, Interstellar Gas, Microwave Emission, X Ray Astronomy

Scientific paper

An attempt is made to show how measurements of X-ray emission from clusters of galaxies combined with measurements of the relative diminution of the cosmic background radiation can be used to determine both the luminosity distance to a cluster and the Hubble constant. Various upper and lower limits to the Hubble constant are computed on the basis of X-ray flux data for several clusters of galaxies. Sources of uncertainty associated with the outlined method are discussed.

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