The Birmingham-CfA cluster scaling project -I. Gas fraction and the M-Tx relation

Monthly Notices of the Royal Astronomical Society

Volumn 340, Issue 3, 2003, Pages 989-1010

  Sanderson, A J R ^a   Ponman, T J ^b   Finoguenov, A ^c   Lloyd Davies, E J ^d   Markevitch, M ^e  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF MICHIGAN   (United States)

^e UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

Author keywords

Galaxies: Clusters: General; Galaxies: Haloes; Intergalactic medium; X rays: Galaxies; X rays: Galaxies: Clusters

Indexed keywords

DENSITY OF GASES; GASES; ISOTHERMS;

BIRMINGHAM; GALAXIES: CLUSTERS: GENERAL; GALAXY:HALO; GAS COOLING; GAS DENSITY; GAS FRACTION; INTERGALACTIC MEDIUM; SCALINGS; X-RAYS GALAXIES CLUSTERS; X-RAYS: GALAXIES;

GALAXIES;

EID: 0141738805     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06401.x     Document Type: Article

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