SAS 3 and related observations of Abell 2029

Details SAS 3 and related observations of Abell 2029 SAS 3 and related observations of Abell 2029

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..738j&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Mar. 15, 1980, p. 738-744. Research supported by the Lockheed Independent Research Pro

Astronomy and Astrophysics

Astronomy

6

Galactic Clusters, Radio Galaxies, Sas-3, Spaceborne Astronomy, X Ray Sources, Ariel 5 Satellite, Heao 1, High Temperature Gases, Intergalactic Media, Oso-8

Scientific paper

X-ray and radio observations of the cluster of galaxies show that the central cD galaxy dominates the emissions. Resolution of the X-ray source shows that its extent is significantly greater than that of the profile of surface brightness of the cD galaxy. Dressler's model of most of the cluster mass with very high M/L(v) is similarly extended. The optically dark mass may provide low-energy X-ray emission of the coronae of 5 x 10 to the 16th stars with very high M/L(v), but in the 2-10 keV range the data are consistent with current theoretical predictions for hot intracluster gas.

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