Comparison of approximately isothermal gravitational potentials of elliptical galaxies based on X-ray and optical data

Monthly Notices of the Royal Astronomical Society

Volumn 404, Issue 3, 2010, Pages 1165-1185

  Churazov, E ^a,b   Tremaine, S ^c   Forman, W ^d   Gerhard, O ^e   Das, P ^e   Vikhlinin, A ^b,d   Jones, C ^d   Bohringer H ^e   Gebhardt, K ^f  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Department of Satellite Monitoring Technologies   (Russian Federation)

^c INSTITUTE FOR ADVANCED STUDY   (United States)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e MPI fur Extraterrestrische Physik   (Germany)

^f UNIVERSITY OF TEXAS AT AUSTIN   (United States)

Author keywords

Galaxies: kinematics and dynamics; X rays: galaxies: clusters

Indexed keywords

GRAVITATION; ISOTHERMS;

CHANDRA; ELLIPTICAL GALAXIES; GALAXIES: KINEMATICS AND DYNAMICS; GRAVITATIONAL POTENTIAL; ISOTHERMAL SPHERES; OPTICAL DATA; THERMAL PRESSURE; X RAY DATA; X-RAYS GALAXIES CLUSTERS; XMM-NEWTON;

GALAXIES;

EID: 77953579320     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16377.x     Document Type: Article

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