R. F. Webbink
- Astronomy and Astrophysics top 0.5%
- Stellar, planetary, and galactic studies 39
- Astrophysical Phenomena and Observations 26
- Gamma-ray bursts and supernovae 20
- Astro and Planetary Science 19
- Astrophysics and Star Formation Studies 15
- Pulsars and Gravitational Waves Research 8
- Instrumentation top 1%
- Astronomy and Astrophysical Research 21
- Geophysics top 10%
- Computational Mechanics top 5%
- Astronomical Observations and Instrumentation 11
R. F. Webbink
62 papers receiving 3.7k citations
Hit Papers
Peers
Comparison fields: 5 of 54
- Astronomy and Astrophysics 3.8k
- Instrumentation 580
- Nuclear and High Energy Physics 389
- Geophysics 192
- Computational Mechanics 198
Countries citing papers authored by R. F. Webbink
This map shows the geographic impact of R. F. Webbink'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 R. F. Webbink with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. F. Webbink more than expected).
Fields of papers citing papers by R. F. Webbink
This network shows the impact of papers produced by R. F. Webbink. 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 R. F. Webbink. The network helps show where R. F. Webbink may publish in the future.
Co-authorship network
The 25 scholars most cited alongside R. F. Webbink, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2024 | 13 | |
| 2 | 2012 | 1 | |
| 3 | 2010 | 7 | |
| 4 | 2010 | 0 | |
| 5 | 2010 | 102 | |
| 6 | 2005 | 61 | |
| 7 | 2004 | 11 | |
| 8 | Contact Binaries | 2003 | 4 |
| 9 | A Self-Consistent Binary Population Synthesis Model | 2001 | 2 |
| 10 | 1990 | 2 | |
| 11 | 1988 | 2 | |
| 12 | Tidal interaction and coalescence of close binary white dwarfs. | 1987 | 3 |
| 13 | 1987 | 3 | |
| 14 | 1983 | 47 | |
| 15 | The Initial Mass Function of White Dwarfs in Cataclysmic Binaries | 1980 | 1 |
| 16 | 1980 | 1 | |
| 17 | 1979 | 3 | |
| 18 | 1979 | 16 | |
| 19 | 1979 | 7 | |
| 20 | The Evolutionary Fate of Contact Binaries | 1975 | 1 |
About R. F. Webbink
R. F. Webbink is a scholar working on Instrumentation, Astronomy and Astrophysics and Computational Mechanics, having authored 65 papers that have together received 3.9k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (39 papers), Astrophysical Phenomena and Observations (26 papers), Astronomy and Astrophysical Research (21 papers), Gamma-ray bursts and supernovae (20 papers), Astro and Planetary Science (19 papers), Astrophysics and Star Formation Studies (15 papers), Astronomical Observations and Instrumentation (11 papers) and Pulsars and Gravitational Waves Research (8 papers). The work is most often cited by research in Astronomy and Astrophysics (3.8k citations), Instrumentation (580 citations) and Nuclear and High Energy Physics (389 citations). R. F. Webbink has collaborated with scholars based in United States, China and Australia. Frequent co-authors include Zhanwen Han, Hongwei Ge, V. Kalogera, Michael M. Shara, S. Rappaport, P. C. Joss, Scott J. Kenyon, R. A. Downes, Xuefei Chen and G. J. Savonije. Their work appears in journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.
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.