Dark Universe: Matter, Energy and Gravity (2004)(en)(204s) by Livio M.

By Livio M.

Number of overview articles on all features of darkish subject and theories of gravity.

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Munn, J. , Nichol, R. , Pier, J. , Schneider, D. , Smith, J. , Winget, D. , York, D. , Anderson, J. , Connolly, A. , Frieman, J. , Gunn, J. , Hennessy, G. , Hindsley, R. , Lamb, D. , Lupton, R. , Newberg, H. , Schlegel, D. , Strauss, M. , Thakar, A. , & Yanny, B. 2001 ApJ 549, L109. , & Guibert, J. 2000 ApJ 532, L41. , Richer, H. , Gilliland, R. , & Scott, D. 1999 ApJ 524, L95. McGrath, E. J. & Sahu, K. C. 09. Monet, D. , Fisher, M. , Harris, H. , & Reid, I. N. 2000 AJ 120, 1541. Oppenheimer, B.

Sanders, R. H. 1991 MNRAS 249, 523. Einstein, A. 1936 Science 84, 506. Evans, E. N. & Eamonn, K. 2000 ApJ 529, 917. Evans, N. , Turner, M. , & Binney, J. 1998 ApJ 501, L45. , & Stark, A. 1989 ApJ 342, 272. Gates, E. L. & Gyuk, G. 2001 ApJ 547, 786. Gould, A. 1994 ApJ 421, L71. Gould, A. 1995 ApJ 441, 77. Graff, D. 2001. In Microlensing 2000: A New Era of Microlensing Astrophysics (eds. J. W. Menzies & Penny D. Sackett). ASP Conference Proceedings, vol. 239, p. 73. ASP. , & Griest, K. 2000 ApJ 535, 90.

X-ray properties of clusters The properties of clusters, their X-ray properties in particular, make them excellent cosmological probes. g. Boldt et al. 1966; Gursky et al. 1971). Images of X-ray clusters span arcminutes, co-spatially with the cluster galaxies. 12h−1 Mpc where the Hubble constant H0 is parameterized as h = H0 /100 km s−1 Mpc−1 . X-ray emission from hot gas has been detected from nearby clusters at projected radii as large as 5 Mpc. The diffuse gas is optically thin at most wavelengths, and therefore derivations of gas masses are not complicated by the effects of radiative transfer.

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