В. И. Шенаврин
About
In The Last Decade
В. И. Шенаврин
95 papers receiving 386 citations
Peers
Comparison fields: 5 of 20
- Astronomy and Astrophysics 398
- Instrumentation 63
- Nuclear and High Energy Physics 42
- Atomic and Molecular Physics, and Optics 23
- Computational Mechanics 21
Countries citing papers authored by В. И. Шенаврин
This map shows the geographic impact of В. И. Шенаврин'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 В. И. Шенаврин with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites В. И. Шенаврин more than expected).
Fields of papers citing papers by В. И. Шенаврин
This network shows the impact of papers produced by В. И. Шенаврин. 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 В. И. Шенаврин. The network helps show where В. И. Шенаврин may publish in the future.
Co-authorship network of co-authors of В. И. Шенаврин
This figure shows the co-authorship network connecting the top 25 collaborators of В. И. Шенаврин. A scholar is included among the top collaborators of В. И. Шенаврин 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 В. И. Шенаврин. В. И. Шенаврин is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 3 | |
| 3 | 4 | |
| 4 | 11 | |
| 5 | 10 | |
| 6 | Hot Dust Revealed During The Dimming Of The T Tau Star RW Aur A | 3 |
| 7 | Infrared activity of the Seyfert galaxy NGC 4151 in 1995-1998 | 1 |
| 8 | Correlation between the infrared and optical variations of NGC 4151 in 30 years: Change in the sizes of the infrared source | 4 |
| 9 | Infrared observations of FG Sagittae in 1993-1997 | 8 |
| 10 | Observations of Sakurai's object (V4334 Sgr) in 1997 and its evolution in 1996-1997 | 3 |
| 11 | Moscow Spectrophotometric Catalog (MSC) (Glushneva+ 1998) | 1 |
| 12 | Nuclear variability of NGC 4151 in UVB and JHKL: A new cycle of activity | 1 |
| 13 | Search for dust shells in W Ser binaries and similar object: RX Cassiopeiae and TX Ursae Majoris | 4 |
| 14 | NGC 4151: Infrared variability | 1 |
| 15 | Photometric JK Observations of Cyg X-1: Binary Parameters from Optical and Infrared Data | 1 |
| 16 | Secondary spectrophotometric standards | 9 |
| 17 | Spectroscopy and Photometry of Nova-Vulpeculae 1984:2 | 1 |
| 18 | The 1953-1984 Bright State of Ry-Tauri - Spectroscopy and Photometry | 1 |
| 19 | The 1983-1984 bright state of RY Tauri: Spectroscopy and photometry | 2 |
| 20 | Kuwano's peculiar object: A nova-like /symbiotic/ binary system containing a red giant - Discussion of observational results | 1 |
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.