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Preprint . 2000
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New Astronomy
Article . 2000 . Peer-reviewed
License: Elsevier TDM
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https://dx.doi.org/10.48550/ar...
Article . 2000
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https://dx.doi.org/10.1016/s13...
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Binary globular clusters

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Sep 2000Embargo end date: 01 Jan 2000 English Publisher:Elsevier BVJournal:New Astronomy, volume 5, pages 349-360 (issn: 1384-1076, Copyright policy )
Authors: Gurzadyan, G. A.;

doi: 10.1016/s1384-1076(00)00028-2 , 10.48550/arxiv.astro-ph/0007225

arXiv: astro-ph/0007225

Binary globular clusters

Abstract

The dynamics of a close binary system of globular clusters is considered. It is shown that the star transfer process from one of the components to the other should lead to the decrease of dimension of the first cluster with simultaneous increase of the dimension of the second cluster. The rates of variations of clusters' sizes due to the mutual tidal interaction between the components, as well as of the orbital rotation of the binary system on the evolution of clusters' sizes, are estimated. The results may be attributed to the double nuclei observed in certain galaxies.

LATEX, 7 .gif figures; to appear in New Astronomy

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
2
Average
Average
Average
Green
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