The baryon mass distribution for nearby galaxy clusters

Astronomy Letters

Volumn 28, Issue 12, 2002, Pages 793-798

  Voevodkin, A A ^a   Vikhlinin, A A ^a   Pavlinsky, M N ^a  

^a Russian Academy of Sciences   (Russian Federation)

Author keywords

Baryon mass function; Galaxy clusters; Large scale structure of the Universe; Theoretical and observational cosmology

Indexed keywords

EID: 0036946375     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1525830     Document Type: Article

References (13)

1. S. Allen, R. Schmidt, and A. Fabian, astro-ph/0205007.
2. S. Buries, K. Nollett, and M. Turner, Astrophys. J. 552, L1 (2001).
3. W. Cash, Astrophys. J. 228, 939 (1979).
4. A. Evrard, T. MacFarland, H. Couchman, et al., Astrophys. J. 573, 7 (2002).
5. A. Fabian, E. Hu, L. Cowie, and J. Grindlay, Astrophys. J. 248, 47(1981).
6. J. Henry, Astrophys. J. 534, 565 (2000).
7. A. Jenkins, C. Frenk, S. White, et al., Mon. Not. R. Astron. Soc. 321, 372 (2001).
8. M. Markevitch, Astrophys. J. 504, 27 (1998).
9. T. Reiprich and H. Bohringer, Astrophys. J. 567, 716 (2002).
10. P. Schechter, Astrophys. J. 203, 297 (1976).
11. A. Vikhlinin, W. Forman, and C. Jones, Astrophys. J. 525, 47 (1999).
12. A. A. Voevodkin, A. A. Vikhlinin, and M. N. Pavlinsky, Pis'ma Astron. Zh. 28, 417 (2002) [Astron. Lett. 28, 366 (2002)].
13. S. White, J. Navarro, A. Evrard, and C. Frenk, Nature 366, 429 (1993).