Milva G. Orsaria
- Astronomy and Astrophysics top 5%
- Geophysics top 5%
- Nuclear and High Energy Physics top 5%
- Atomic and Molecular Physics, and Optics
- Oceanography
- Co-authors
- Gustavo A. ContreraFridolin WeberIgnacio F. Ranea‐SandovalMauro MarianiH. RodriguesA. Pérez Martı́nezN. N. ScoccolaHugo Pérez Rojas
- Topics
- Pulsars and Gravitational Waves Research (35 papers)High-pressure geophysics and materials (23 papers)Gamma-ray bursts and supernovae (17 papers)
- Journals
- The Astrophysical JournalMonthly Notices of the Royal Astronomical SocietyPhysical review. D
- Partner nations
- ArgentinaUnited StatesBrazil
In The Last Decade
Milva G. Orsaria
37 papers receiving 700 citations
Peers
Comparison fields: 5 of 15
- Astronomy and Astrophysics 637
- Geophysics 282
- Nuclear and High Energy Physics 256
- Atomic and Molecular Physics, and Optics 123
- Oceanography 54
Countries citing papers authored by Milva G. Orsaria
This map shows the geographic impact of Milva G. Orsaria'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 Milva G. Orsaria with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Milva G. Orsaria more than expected).
Fields of papers citing papers by Milva G. Orsaria
This network shows the impact of papers produced by Milva G. Orsaria. 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 Milva G. Orsaria. The network helps show where Milva G. Orsaria may publish in the future.
Co-authorship network of co-authors of Milva G. Orsaria
This figure shows the co-authorship network connecting the top 25 collaborators of Milva G. Orsaria. A scholar is included among the top collaborators of Milva G. Orsaria 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 Milva G. Orsaria. Milva G. Orsaria 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 | 7 | |
| 3 | 29 | |
| 4 | 1 | |
| 5 | 2 | |
| 6 | 1 | |
| 7 | 23 | |
| 8 | 14 | |
| 9 | Hybrid magnetized stars within the Field Correlator Method | 1 |
| 10 | 48 | |
| 11 | 9 | |
| 12 | 19 | |
| 13 | Hybrid Stars in the Framework of NJL Models | 1 |
| 14 | 2 | |
| 15 | 12 | |
| 16 | 17 | |
| 17 | 56 | |
| 18 | 3 | |
| 19 | 5 | |
| 20 | 0 |
About Milva G. Orsaria
Milva G. Orsaria is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics, having authored 41 papers that have together received 714 indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (35 papers), High-pressure geophysics and materials (23 papers) and Gamma-ray bursts and supernovae (17 papers). The work is most often cited by research in Astronomy and Astrophysics (637 citations), Geophysics (282 citations) and Nuclear and High Energy Physics (256 citations). Milva G. Orsaria has collaborated with scholars based in Argentina, United States and Brazil. Frequent co-authors include Gustavo A. Contrera, Fridolin Weber, Ignacio F. Ranea‐Sandoval, Mauro Mariani, H. Rodrigues, A. Pérez Martı́nez, N. N. Scoccola, Hugo Pérez Rojas, O. M. Guilera and R. González Felipe. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Physical review. D.
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.