O. G. Benvenuto
- Astronomy and Astrophysics top 1%
- Nuclear and High Energy Physics top 5%
- Geophysics top 5%
- Instrumentation top 5%
- Atomic and Molecular Physics, and Optics top 10%
- Co-authors
- L. G. AlthausJ. E. HorvathG. LugonesAldo SerenelliH. VucetichA. BruniniK. NomotoMelina C. Bersten
- Topics
- Stellar, planetary, and galactic studies (57 papers)Pulsars and Gravitational Waves Research (56 papers)Gamma-ray bursts and supernovae (31 papers)
In The Last Decade
O. G. Benvenuto
103 papers receiving 1.8k citations
Peers
Comparison fields: 5 of 41
- Astronomy and Astrophysics 1.8k
- Nuclear and High Energy Physics 499
- Geophysics 281
- Instrumentation 218
- Atomic and Molecular Physics, and Optics 203
Countries citing papers authored by O. G. Benvenuto
This map shows the geographic impact of O. G. Benvenuto'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 O. G. Benvenuto with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. G. Benvenuto more than expected).
Fields of papers citing papers by O. G. Benvenuto
This network shows the impact of papers produced by O. G. Benvenuto. 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 O. G. Benvenuto. The network helps show where O. G. Benvenuto may publish in the future.
Co-authorship network of co-authors of O. G. Benvenuto
This figure shows the co-authorship network connecting the top 25 collaborators of O. G. Benvenuto. A scholar is included among the top collaborators of O. G. Benvenuto 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 O. G. Benvenuto. O. G. Benvenuto is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 6 | |
| 3 | 3 | |
| 4 | 1 | |
| 5 | 1 | |
| 6 | 3 | |
| 7 | 4 | |
| 8 | Early ultraviolet/optical emission of the type Ib SN 2008D | 20 |
| 9 | 17 | |
| 10 | 28 | |
| 11 | 25 | |
| 12 | 39 | |
| 13 | 2 | |
| 14 | Formation and Evolution of a 0. 242 M ☉ Helium White Dwarf in Presence of Element Diffusion | 1 |
| 15 | 16 | |
| 16 | Formation and Evolution of a 0.242 M ⊙ Helium White Dwarf in Presence of Element Diffusion | 16 |
| 17 | 1 | |
| 18 | Optical study of LMXBs with high temporal resolution: evidence for non-thermal flares from MXB 1735-44. | 1 |
| 19 | Improvements on the structure of strange stars | 4 |
| 20 | On the planetary nebula NGC 3918. | 3 |
About O. G. Benvenuto
O. G. Benvenuto is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 108 papers that have together received 1.9k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (57 papers), Pulsars and Gravitational Waves Research (56 papers) and Gamma-ray bursts and supernovae (31 papers). The work is most often cited by research in Astronomy and Astrophysics (1.8k citations), Instrumentation (218 citations) and Nuclear and High Energy Physics (499 citations). O. G. Benvenuto has collaborated with scholars based in Argentina, Brazil and Chile. Frequent co-authors include L. G. Althaus, J. E. Horvath, G. Lugones, Aldo Serenelli, H. Vucetich, A. Brunini, K. Nomoto, Melina C. Bersten, R. D. Rohrmann and A. Fortier. Their work appears in journals such as Physical Review Letters, 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.