Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-05-21
Bull.Spec.Astrophys.Obs.N.Caucasus 58:5-15,2005
Astronomy and Astrophysics
Astrophysics
11 pages, 8 figures
Scientific paper
From photometric observations of elliptical galaxies, among which are both radio galaxies and radio-quiet objects, an investigation was carried out of the relationship `redshift -- age of the stellar system' $(\Delta z/\Delta t)$. By means of this relationship cosmological parameters $H(z)$ and $\Omega_\Lambda$ are estimated. Ages of stellar systems are determined within the framework of evolution models of synthetic spectra PEGASE and GISSEL. This approach can be considered as time study of objects of the early Universe independent of other cosmological models. Construction of a pooled sample is described, containing 220 objects from different populations of elliptical galaxies, for which an analysis of the upper limit of the age of formation of a stellar system was performed. These data were used to estimate the boundaries of determination of the cosmological parameters $H_0$ and $\Lambda$--term: $H_0=72\pm10$ and $\Omega_\Lambda=0.8\pm0.1$ in the model GISSEL and $H_0=53\pm10$, and $\Omega_\Lambda=0.8\pm0.1$ in the model PEGASE.
Parijskij Yu. N.
Starobinsky Alexei A.
Verkhodanov Oleg V.
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