В. С. Шевченко
About
In The Last Decade
В. С. Шевченко
41 papers receiving 513 citations
Peers
Comparison fields: 5 of 20
- Astronomy and Astrophysics 514
- Spectroscopy 65
- Instrumentation 36
- Computational Mechanics 18
- Atmospheric Science 17
Countries citing papers authored by В. С. Шевченко
This map shows the geographic impact of В. С. Шевченко'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. С. Шевченко with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites В. С. Шевченко more than expected).
Fields of papers citing papers by В. С. Шевченко
This network shows the impact of papers produced by В. С. Шевченко. 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. С. Шевченко. The network helps show where В. С. Шевченко may publish in the future.
Co-authorship network of co-authors of В. С. Шевченко
This figure shows the co-authorship network connecting the top 25 collaborators of В. С. Шевченко. A scholar is included among the top collaborators of В. С. Шевченко 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. С. Шевченко. В. С. Шевченко is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 121 | |
| 2 | 11 | |
| 3 | V380 Ori--A Herbig Ae/Be star at an early stage of envelope formation: Hydrogen-line profiles | 2 |
| 4 | The quasi-Algol GW Ori: The nature of eclipses and estimation of the component masses | 4 |
| 5 | Radial velocity of the protoalgol BM Ori | 1 |
| 6 | HD 216629=IL Cep, BHJ 71, and LkH alpha 350--Probable Herbig Ae/Be stars in the Cep OB3 association: HD 216629 AB and LkH alpha 350 | 4 |
| 7 | On the Periodicity of WA CrA/1 and WA CrA/2 WTTS | 1 |
| 8 | Photometric study of the properties of SPOT rotational modulation in weak line T Tauri stars. | 1 |
| 9 | HD 216629-IL Cep, BHJ 71, and LkH alpha 350-Probable Ae/Be Herbig stars in the association Cep OB3: The association Cep OB3 and BHJ 71 | 1 |
| 10 | V380 ORI : an Ae/Be Herbig star at an early stage of the envelope formation. Emission lines of metal. | 1 |
| 11 | V380 Ori: An Ae/Be Herbig star at an early stage of its envelope formation-emission lines of metals | 1 |
| 12 | UBVR monitoring of HZ Her=Her X-1: On shape variability of the accretion region and of the hot spot in the subgiant photosphere | 1 |
| 13 | Photometric and spectroscopic observations of the spotted T Tauri star V410 Tauri. | 3 |
| 14 | Compact Star-Formation Regions Associated with the Herbig Ae-Stars / Be-Stars LK-H-ALPHA:198 and LK-H-ALPHA:234 | 8 |
| 15 | The compact star forming regions associated with Herbig Ae/Be stars LK H-alpha 198 and LK H-alpha 234. | 1 |
| 16 | Variabilility of the Herbig Be star BHJ 71 | 1 |
| 17 | BM Orionis : the unique eclipsing binary in the Trapezium. The components and extended matter round the cool star. I. Photoelectric observations. | 1 |
| 18 | The light curve of HZ Herculis near minimum, and an interpretation | 0 |
| 19 | The structure of star formation regions I. Population categories and the evolution of molecular clouds | 1 |
| 20 | On the possibility of nuclear explosion in a contracting protostar. | 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.