The cluster gas mass fraction as a cosmological probe: A revised study

Astronomy and Astrophysics

Volumn 501, Issue 1, 2009, Pages 61-73

  Ettori, S ^a,b   Morandi, A ^c,d   Tozzi, P ^e,f   Balestra, I ^g   Borgani, S ^e,f,h   Rosati, P ⁱ   Lovisari, L ^c,j   Terenziani, F ^c  

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b INFN SEZIONE DI BOLOGNA   (Italy)

^c UNIVERSITY OF BOLOGNA   (Italy)

^d UNIVERSITY OF COPENHAGEN   (Denmark)

^e INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^f SEZIONE DI TRIESTE   (Italy)

^g MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^h UNIVERSITY OF TRIESTE   (Italy)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^j UNIVERSITY OF INNSBRUCK   (Austria)

more..

Author keywords

Cosmology: observations; Dark matter; Galaxies: clusters: general; Galaxies: fundamental parameters; Intergalactic medium; X rays: galaxies: clusters

Indexed keywords

COSMOLOGY: OBSERVATIONS; DARK MATTER; GALAXIES: CLUSTERS: GENERAL; GALAXIES: FUNDAMENTAL PARAMETERS; INTERGALACTIC MEDIUM; X-RAYS: GALAXIES: CLUSTERS;

BUDGET CONTROL; COSMIC RAY MEASUREMENT; COSMOLOGY; FERMIONS; GALAXIES; GASES; SIGNAL TO NOISE RATIO; STARS; X RAYS;

DENSITY OF GASES;

EID: 67650909563     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810878     Document Type: Article

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