A new method to estimate cosmological parameters using the baryon fraction of clusters of galaxies

Publications of the Astronomical Society of Japan

Volumn 48, Issue 6, 1996, Pages

  Sasaki, Shin ^a  

^a TOKYO METROPOLITAN UNIVERSITY   (Japan)

Author keywords

Cosmology; Galaxies: Clusters of; X rays

Indexed keywords

GALAXIES; HADRONS;

CLUSTER OF GALAXIES; COSMOLOGICAL PARAMETERS; GALAXIES CLUSTERS; GALAXY: CLUSTER OF; RED SHIFT; THEORETICAL CALCULATIONS;

COSMOLOGY;

EID: 0030299431     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/48.6.L119     Document Type: Article

References (8)

1. Buote D.A., Canizares C.R. 1996, ApJ 457, 565
2. Neumann D.M., Böhringer H. 1996, MNRAS in press
3. Peebles P.J.E. 1993, Principles of Physical Cosmology (Princeton University Press, New Jersey)
4. Rybicki G.B., Lightman A.P. 1979, Radiative Processes in Astrophysics (Wiley, New York)
5. Sarazin C.L. 1988, X-ray emission from clusters of galaxies (Cambridge University Press, Cambridge)
6. Squires G., Kaiser N., Babul A., Fahlman G., Woods D., Neumann D.M., Böhringer H. 1996, ApJ 461, 572
7. White D.A., Fabian A.C. 1995, MNRAS 273, 72
8. White S.D.M., Navarro J.F., Evrard A.E., Frenk C.S. 1993, Nature 366, 429