Why are rotating elliptical galaxies less elliptical at X-ray frequencies?

Astrophysical Journal

Volumn 539, Issue 2 PART 1, 2000, Pages 675-686

  Brighenti, Fabrizio ^a,b   Mathews, William G ^a  

^a University of California Santa Cruz   (United States)

^b UNIVERSITY OF BOLOGNA   (Italy)

Author keywords

Cooling flows; Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: ISM; X rays: galaxies

Indexed keywords

EID: 0034691977     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309266     Document Type: Article

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