Citations per year, relative to N. I. Shakura N. I. Shakura (= 1×)
peers
A. P. Smale
Countries citing papers authored by N. I. Shakura
Since
Specialization
Citations
This map shows the geographic impact of N. I. Shakura'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 N. I. Shakura with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites N. I. Shakura more than expected).
This network shows the impact of papers produced by N. I. Shakura. 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 N. I. Shakura. The network helps show where N. I. Shakura may publish in the future.
Co-authorship network of co-authors of N. I. Shakura
This figure shows the co-authorship network connecting the top 25 collaborators of N. I. Shakura.
A scholar is included among the top collaborators of N. I. Shakura 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 N. I. Shakura. N. I. Shakura is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Постнов, К. А., N. I. Shakura, A. Kochetkova, & L. Hjalmarsdotter. (2014). Do we see accreting magnetars in X-ray pulsars?. Springer Link (Chiba Institute of Technology).7 indexed citations
Staubert, R., D. Klochkov, К. А. Постнов, et al.. (2013). VizieR Online Data Catalog: Her X-1 pulse profiles (Staubert+, 2013).
8.
Klochkov, D., R. Staubert, К. А. Постнов, et al.. (2008). INTEGRAL observations of Hercules X-1. Springer Link (Chiba Institute of Technology).27 indexed citations
9.
Shakura, N. I. & R. Sunyaev. (1999). The Physics of Turbulent Boundary Layer. 38. 197.1 indexed citations
10.
Shakura, N. I., et al.. (1999). HER X-1: a New Model for X-Ray Dips. 38. 165.1 indexed citations
11.
Shakura, N. I., К. А. Постнов, & М. Е. Прохоров. (1991). Presence of a Quadrupole Component of the Magnetic Field Near the Surface of the Neutron Star in HERCULES-X-1. 17. 339.
12.
Shakura, N. I.. (1987). Geodesics in a Kerr Metric. 13. 99.1 indexed citations
13.
Syunyaev, R. A. & N. I. Shakura. (1986). Disk Accretion onto a Weak Field Neutron Star - Boundary Layer Disk Luminosity Ratio. 12. 117–120.
14.
Shakura, N. I.. (1985). On the apsidal motion in binary stars. 11. 224–226.3 indexed citations
15.
Lipunov, V., et al.. (1981). Accretion disk orientation in binary X-ray pulsars. Астрономический журнал. 58. 765–770.2 indexed citations
16.
Lipunov, V. & N. I. Shakura. (1976). On the nature of binary-system x-ray pulsars. 2. 133–135.
17.
Lipunov, V. & N. I. Shakura. (1976). On the nature of binary X-ray pulsars.. 2. 343–348.
18.
Shakura, N. I.. (1975). The X-ray pulsar 3U 0900-40 with long period - a neutron star with anomalously strong magnetic field.. 1. 23–28.
19.
Shakura, N. I.. (1975). The long-period x-ray pulsar 3U 0900--40 as a neutron star with an abnormally strong magnetic field. 1. 223–225.3 indexed citations
20.
Cherepashchuk, A. M., et al.. (1972). On the Nature of the Optical Variations of HZ Her = Her X1. Information Bulletin on Variable Stars. 720(720). 1.2 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.