Countries citing papers authored by V. L. Polyachenko
Since
Specialization
Citations
This map shows the geographic impact of V. L. Polyachenko's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by V. L. Polyachenko with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites V. L. Polyachenko more than expected).
Fields of papers citing papers by V. L. Polyachenko
This network shows the impact of papers produced by V. L. Polyachenko. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by V. L. Polyachenko. The network helps show where V. L. Polyachenko may publish in the future.
Co-authorship network of co-authors of V. L. Polyachenko
This figure shows the co-authorship network connecting the top 25 collaborators of V. L. Polyachenko.
A scholar is included among the top collaborators of V. L. Polyachenko based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with V. L. Polyachenko. V. L. Polyachenko is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Fridman, A. M., O. V. Khoruzhii, E. V. Polyachenko, et al.. (2001). New Structures in Galactic Disks: Predictions and Discoveries. University of Hertfordshire Research Archive (University of Hertfordshire). 230. 187–198.3 indexed citations
8.
Polyachenko, V. L., et al.. (1997). Stability criteria for gaseous self-gravitating disks. Astronomy Letters. 23. 483.12 indexed citations
9.
Polyachenko, V. L. & E. V. Polyachenko. (1996). Formation of slow bars in early-type spiral galaxies. Astronomy Letters. 22(3). 302–308.1 indexed citations
10.
Polyachenko, V. L. & E. V. Polyachenko. (1994). Galactic slow bar as an unstable mode of a stellar disk. Astronomy Letters. 20(4). 416–423.2 indexed citations
11.
Polyachenko, V. L.. (1992). Theory of Bars in Disk Shaped Galaxies as Aligned Orbits. 36. 5.1 indexed citations
12.
Fridman, A. M., V. L. Polyachenko, & A. V. Zasov. (1991). On Some Observational Restrictions to Galactic Spiral Structure Theories. 146. 109.1 indexed citations
13.
Gorkavyi, Nick, V. L. Polyachenko, & A. M. Fridman. (1990). Dissipative instability of the protoplanetary disk and the law of planetary distances. 16. 183–190.2 indexed citations
14.
Nezlin, M. V., et al.. (1986). Interarm Vortices Predicted by Laboratory Simulation of Spiral Structure. 12. 213–219.4 indexed citations
15.
Fridman, A. M. & V. L. Polyachenko. (1984). Physics of Gravitating Systems II. CERN Document Server (European Organization for Nuclear Research).47 indexed citations
16.
Polyachenko, V. L. & I. G. Shukhman. (1982). Collisions in Spherical Stellar Systems. Soviet Astronomy. 26. 140–145.1 indexed citations
17.
Polyachenko, V. L. & I. G. Shukhman. (1981). General Models of Collisionless Spherically Symmetric Stellar Systems - a Stability Analysis. 25. 533.27 indexed citations
18.
Polyachenko, V. L., S. M. Churilov, & I. G. Shukhman. (1980). The nonlinear stage of gravitational instability in flat gaseous systems. 24. 287–291.
19.
Polyachenko, V. L. & A. M. Fridman. (1972). LAW OF PLANETARY DISTANCES.. AZh. 16. 123.1 indexed citations
20.
Ginzburg, I.F., V. L. Polyachenko, & A. M. Fridman. (1971). Ring Stability of Saturn.. Astronomicheskii Zhurnal. 15. 643.4 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.