Galaxy merging and number vs. apparent magnitude relation for the universe with a time-decaying cosmological term

Astronomy and Astrophysics

Volumn 449, Issue 3, 2006, Pages 903-916

  Komiya, Z ^a   Kawabata, K ^a   Hirano, K ^a   Bunya, H ^a   Yamamoto, N ^b  

^a TOKYO UNIVERSITY OF SCIENCE   (Japan)

^b NATIONAL INSTITUTE OF ADVANCED INDUSTRIAL SCIENCE AND TECHNOLOGY AIST   (Japan)

Author keywords

Cosmic microwave background; Cosmological parameters; Galaxy: general

Indexed keywords

GALAXIES; MICROWAVES; NUMERICAL METHODS; STATISTICAL METHODS;

COSMIC MICROWAVE BACKGROUND RADIATION (CMBR) SPECTRUM; HUBBLE PARAMETER;

ASTROPHYSICS;

EID: 33645706575     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054406     Document Type: Article

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