Non-Linear Cosmology of Globular Cluster Systems around Galaxies

Authors

  • I. U. Tadjibaev National University of Uzbekistan (2, Universitetskaya Str., Tashkent, Uzbekistan)
  • S. N. Nuritdinov National University of Uzbekistan (2, Universitetskaya Str., Tashkent, Uzbekistan)
  • A. A. Muminov National University of Uzbekistan (2, Universitetskaya Str., Tashkent, Uzbekistan)

DOI:

https://doi.org/10.15407/ujpe62.12.1057

Keywords:

systems of globular star clusters, gravitational instabilities, pulsation model of self-gravitating system, cosmology of globular clusters

Abstract

The formation of systems of globular star clusters around galaxies has been studied in the framework of a nonlinear-nonstationary model of collapsing galaxies. Instabilities of the model with respect to four perturbation modes are analyzed, with the mode order determining the average number of clusters in the system. Critical diagrams for the dependence of the initial value of the virial ratio on the rotation degree of collapsing model are plotted. The instability growth rates are calculated, and the obtained instability parameters are compared.

UJP 2017 V62 #12

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Published

2018-09-18

Issue

Vol. 62 No. 12 (2017)

Section

Astrophysics and cosmology

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How to Cite

Non-Linear Cosmology of Globular Cluster Systems around Galaxies. (2018). Ukrainian Journal of Physics, 62(12), 1057. https://doi.org/10.15407/ujpe62.12.1057

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