The distance to Hydra and Centaurus from surface brightness fluctuations: Consequences for the Great Attractor model

Astronomy and Astrophysics

Volumn 438, Issue 1, 2005, Pages 103-119

  Mieske, S ^a,b   Hilker, M ^a   Infante, L ^b  

^a UNIVERSITY OF BONN   (Germany)

^b PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

Author keywords

Cosmology: large scale structure of Universe; Galaxies: clusters: individual: Hydra cluster; Galaxies: distances and redshift; Galaxies: kinematics and dynamics; Techniques: photometric

Indexed keywords

ASTROPHYSICS; COSMIC RAYS; DATA REDUCTION; KINEMATICS; MICROWAVES; PHOTOMETRY;

COSMOLOGY: LARGE SCALE STRUCTURE OF UNIVERSE; GALAXIES: CLUSTER: INDIVIDUAL; GALAXIES: DISTANCES AND REDSHIFT; GALAXIES: KINEMATICAL AND DYNAMICS; HYDRA CLUSTERS; TECHNIQUES: PHOTOMETRIC;

GALAXIES;

EID: 23044444805     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041583     Document Type: Article

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