S. M. Ruciński
About
In The Last Decade
S. M. Ruciński
194 papers receiving 4.4k citations
Peers
Comparison fields: 5 of 61
- Astronomy and Astrophysics 4.5k
- Instrumentation 1.5k
- Computational Mechanics 300
- Geophysics 164
- Atomic and Molecular Physics, and Optics 157
Countries citing papers authored by S. M. Ruciński
This map shows the geographic impact of S. M. Ruciński'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 S. M. Ruciński with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. M. Ruciński more than expected).
Fields of papers citing papers by S. M. Ruciński
This network shows the impact of papers produced by S. M. Ruciński. 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 S. M. Ruciński. The network helps show where S. M. Ruciński may publish in the future.
Co-authorship network of co-authors of S. M. Ruciński
This figure shows the co-authorship network connecting the top 25 collaborators of S. M. Ruciński. A scholar is included among the top collaborators of S. M. Ruciński 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 S. M. Ruciński. S. M. Ruciński is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 0 | |
| 3 | MOST photometry and DDO spectroscopy of the eclipsing (white dwarf + red dwarf) binary V471 Tau | 7 |
| 4 | Nonradial p-modes in the G9.5 giant [epsilon] Ophiuchi? Pulsation model fits to MOST photometry | 8 |
| 5 | The Clusters AgeS Experiment (CASE). VI. Analysis of Two Detached Eclipsing Binaries in the Globular Cluster M55 | 1 |
| 6 | 2 | |
| 7 | 11 | |
| 8 | 39 | |
| 9 | On the name "over-contact binary systems" | 1 |
| 10 | Absolute Magnitude Calibration for the W UMa-type Contact Binary Stars | 1 |
| 11 | New results on contact systems in stellar clusters. | 1 |
| 12 | Linear and quadratic limb-darkening coefficients for a large grid of LTE model atmospheres. | 12 |
| 13 | The rate of the angular-momentum loss due to magnetic breaking, as derived from binary statistics | 7 |
| 14 | HD 36705 - a Post T Tauri Star | 1 |
| 15 | A note on the existence of W UMa-type systems in the cluster CR 359. | 0 |
| 16 | Sizes of spots in spotted stars. | 4 |
| 17 | The W UMa-type systems as contact binaries. Pt. 2. A- and W-type systems | 4 |
| 18 | Binaries. II. A- and W-type Systems. The W UMa-type Systems as Contact | 8 |
| 19 | The W UMa-type Systems as Contact Binaries. I. Two Methods of Geometrical Elements Determination. Degree of Contact | 29 |
| 20 | The Eclipsing Binary System DI Pegasi | 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.