... 31 . Renzini A. (1998) in The Young Universe , eds. S. D'Odorico et al. , p. 298 . 32 . ... 1992) A&AS, 96, p.269 . 34 . Shanks T. et al. (1998) in The Young Universe , eds. S. D'Odorico et al. , p.102 . 35 . ...
... gravitational waves from the local galaxy universe" . ... and the equation of state of the universe" . Gromov A., Baryshev Yu., ... and pairwise velocity dispersion in a \Omega=1 universe" . ...
... of high-z galaxies Distance between galaxies in expanding Universe changes as 1 1+z ... How does surface brightness depend on distance in a Euclidean static universe ... In the expanding Universe Io z=1 z=5 µ 3.m 0, µ 8.m 0. bs = Itrue . ...
... of galaxies in the nearby volume of the Universe is highly inhomogeneous ... determining the density fluctuations in the Universe as a function of the scale of ... The LF allows estimating the mean luminosity density in the Universe. ...
... gave rise to a picture of the Universe where the Milky Way is an ordinary stellar ... faint nebulae, it became clear that the Universe is much larger than had previously ...
... Kholtygin A.F. UV lines in spectra of Planetary Nebulae (in russian) , Ultravililet Universe II , Proc. of the Conference, held in Instititute of Astronomy, May 19-20, 2006, Moscow, Eds: B.M.Shustov, M.E.Sachkov, E.A.Kilpio, M., Yanus-K, pp. ...
... Kholtygin A.F. UV lines in spectra of Planetary Nebulae (in russian) , Ultravililet Universe II , Proc. of the Conference, held in Instititute of Astronomy, May 19-20, 2006, Moscow, Eds: B.M.Shustov, M.E.Sachkov, E.A.Kilpio, M., Yanus-K, pp. ...