The XMM-Ω project II. Cosmological implications from the high redshift L - T relation of X-ray clusters

Astronomy and Astrophysics

Volumn 412, Issue 2, 2003, Pages

  Vauclair, S C ^a   Blanchard, A ^a   Sadat, R ^a   Barlett, J G ^b,g   Bernard, J P ^c   Boer, M ^c   Giard, M ^c   Lumb, D H ^d   Marty, P ^e   Nevalainen, J ^f  

^a CNRS   (France)

^b UNIVERSITÉ PARIS DESCARTES   (France)

^c IRAP   (France)

^d EUROPEAN SPACE AGENCY   (Netherlands)

^e UNIVERSITÉ PARIS SUD   (France)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g OBSERVATOIRE DE STRASBOURG   (France)

Author keywords

Cosmological parameters; Cosmology; Dark matter; Galaxies: Clusters: General

Indexed keywords

ATMOSPHERIC TEMPERATURE; EXTRATERRESTRIAL ATMOSPHERES; GALAXIES; MATHEMATICAL MODELS; STATISTICAL METHODS; X RAYS;

COSMOLOGY; POISSONIAN STATISTICS; TEMPERATURE DISTRIBUTION FUNCTION; TEMPERATURE-LUMINOSITY RELATION;

ASTROPHYSICS;

EID: 10744233201     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034603     Document Type: Letter

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