A. Chieffi
- Instrumentation top 0.5%
- Astronomy and Astrophysical Research 27
- Astronomy and Astrophysics top 0.5%
- Stellar, planetary, and galactic studies 66
- Astro and Planetary Science 43
- Gamma-ray bursts and supernovae 41
- Astrophysics and Star Formation Studies 26
- Astrophysical Phenomena and Observations 6
-
- Nuclear physics research studies 16
- Astronomical and nuclear sciences 12
- Radiation top 5%
- Geophysics top 10%
A. Chieffi
83 papers receiving 4.2k citations
Hit Papers
Peers
Comparison fields: 5 of 53
- Instrumentation 1.1k
- Astronomy and Astrophysics 4.0k
- Nuclear and High Energy Physics 1.3k
- Radiation 195
- Geophysics 113
Countries citing papers authored by A. Chieffi
This map shows the geographic impact of A. Chieffi'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 A. Chieffi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Chieffi more than expected).
Fields of papers citing papers by A. Chieffi
This network shows the impact of papers produced by A. Chieffi. 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 A. Chieffi. The network helps show where A. Chieffi may publish in the future.
Co-authorship network
The 25 scholars most cited alongside A. Chieffi, 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 | 2025 | 0 | |
| 2 | 2025 | 0 | |
| 3 | 2025 | 2 | |
| 4 | 2025 | 6 | |
| 5 | 2024 | 0 | |
| 6 | 2023 | 31 | |
| 7 | 2021 | 18 | |
| 8 | 2021 | 12 | |
| 9 | 2021 | 14 | |
| 10 | 2016 | 58 | |
| 11 | Why Do Low-Mass Stars Become Red Giants? | 2012 | 9 |
| 12 | Radioactivites in Low- and Intermediate-Mass Stars | 2011 | 2 |
| 13 | 2009 | 31 | |
| 14 | Presupernova evolution and explosion of massive stars: the role of mass loss during the Wolf-Rayet stage. | 2009 | 0 |
| 15 | 2008 | 2 | |
| 16 | Nucleosynthesis of 60 Fe in massive stars | 2005 | 10 |
| 17 | 2004 | 5 | |
| 18 | 2002 | 115 | |
| 19 | 2001 | 30 | |
| 20 | CNO self-pollution in globular clusters; a model and its possible observational tests. | 1983 | 2 |
About A. Chieffi
A. Chieffi is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 91 papers that have together received 4.4k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (66 papers), Astro and Planetary Science (43 papers), Gamma-ray bursts and supernovae (41 papers), Astronomy and Astrophysical Research (27 papers), Astrophysics and Star Formation Studies (26 papers), Nuclear physics research studies (16 papers), Astronomical and nuclear sciences (12 papers) and Astrophysical Phenomena and Observations (6 papers). The work is most often cited by research in Instrumentation (1.1k citations), Astronomy and Astrophysics (4.0k citations) and Nuclear and High Energy Physics (1.3k citations). A. Chieffi has collaborated with scholars based in Italy, Australia and Japan. Frequent co-authors include Marco Limongi, O. Straniero, M. Salaris, R. Gallino, M. Busso, C. Arlandini, V. Castellani, Maria Lugaro, C. Abia and C. Travaglio. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Supplement Series, Nuclear Physics A and The Astronomical Journal.
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.