The detection of extended X-ray emission surrounding cD galaxies in poor clusters

Details The detection of extended X-ray emission surrounding cD galaxies in poor clusters The detection of extended X-ray emission surrounding cD galaxies in poor clusters

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l..61k&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Jan. 15, 1980, p. L61-L65.

Astronomy and Astrophysics

Astrophysics

46

Astrophysics, Galactic Clusters, X Ray Sources, Intergalactic Media, Red Shift

Scientific paper

The paper presents some preliminary results of a survey, performed with an imaging proportional counter, to detect X-ray emission from poor clusters which nevertheless contain dominant D or cD galaxies and could, therefore, be classified as Bautz-Morgan Type I. The data suggest that poor clusters can collect enough gas to become detectable X-ray sources if they are relatively compact, which the presence of dominant galaxies indicates.

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