X-Ray Emission from Poor Clusters with Dominant Galaxies: Morphology and Evidence for Accretion

Details X-Ray Emission from Poor Clusters with Dominant Galaxies: Morphology and Evidence for Accretion X-Ray Emission from Poor Clusters with Dominant Galaxies: Morphology and Evidence for Accretion

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baas...14r.907c&link_type=gif

Bulletin of the American Astronomical Society, Vol. 14, p.907

Astronomy and Astrophysics

Astronomy

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