A. Chieffi

7.5k total citations · 2 hit papers
91 papers, 4.4k citations indexed

About

A. Chieffi is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, A. Chieffi has authored 91 papers receiving a total of 4.4k indexed citations (citations by other indexed papers that have themselves been cited), including 85 papers in Astronomy and Astrophysics, 27 papers in Instrumentation and 27 papers in Nuclear and High Energy Physics. Recurrent topics in A. Chieffi's work include Stellar, planetary, and galactic studies (66 papers), Astro and Planetary Science (43 papers) and Gamma-ray bursts and supernovae (41 papers). A. Chieffi is often cited by papers focused on Stellar, planetary, and galactic studies (66 papers), Astro and Planetary Science (43 papers) and Gamma-ray bursts and supernovae (41 papers). A. Chieffi collaborates with scholars based in Italy, Australia and Japan. A. Chieffi's co-authors include Marco Limongi, O. Straniero, M. Salaris, R. Gallino, M. Busso, C. Arlandini, V. Castellani, Maria Lugaro, C. Abia and C. Travaglio and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

A. Chieffi

83 papers receiving 4.2k citations

Hit Papers

Evolution and Nucleosynthesis in Low‐Mass Asymptotic Gian... 1998 2026 2007 2016 1998 2018 100 200 300 400 500

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
A. Chieffi Italy 32 4.0k 1.3k 1.1k 195 190 91 4.4k
Marco Limongi Italy 31 3.5k 0.9× 1.3k 1.0× 845 0.8× 231 1.2× 190 1.0× 125 4.0k
Nikos Prantzos France 32 3.8k 1.0× 1.2k 0.9× 1.1k 1.0× 145 0.7× 193 1.0× 119 4.3k
Falk Herwig United States 39 4.3k 1.1× 1.2k 0.9× 983 0.9× 219 1.1× 155 0.8× 131 4.7k
Amanda I. Karakas Australia 41 5.0k 1.3× 1.1k 0.8× 1.5k 1.4× 145 0.7× 165 0.9× 178 5.3k
Ann Merchant Boesgaard United States 29 2.7k 0.7× 832 0.6× 781 0.7× 100 0.5× 202 1.1× 108 3.1k
Raphaël Hirschi United Kingdom 38 6.2k 1.6× 1.1k 0.8× 1.8k 1.7× 124 0.6× 158 0.8× 127 6.6k
S. Cristallo Italy 28 2.3k 0.6× 793 0.6× 520 0.5× 148 0.8× 109 0.6× 104 2.6k
Hideyuki Umeda Japan 35 5.8k 1.5× 1.5k 1.1× 989 0.9× 62 0.3× 156 0.8× 115 6.1k
Wako Aoki Japan 42 5.3k 1.3× 1.2k 0.9× 1.9k 1.8× 223 1.1× 268 1.4× 188 5.8k
Maria Lugaro Australia 32 4.2k 1.1× 1.6k 1.2× 724 0.7× 359 1.8× 187 1.0× 155 4.8k

Countries citing papers authored by A. Chieffi

Since Specialization
Citations

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

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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 of co-authors of A. Chieffi

This figure shows the co-authorship network connecting the top 25 collaborators of A. Chieffi. A scholar is included among the top collaborators of A. Chieffi 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 A. Chieffi. A. Chieffi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Best, A., C. R. Brune, A. Chieffi, et al.. (2025). The $$^{12}$$C$$(\alpha ,\gamma )^{16}$$O reaction, in the laboratory and in the stars. The European Physical Journal A. 61(4).
2.
Limongi, Marco, et al.. (2025). The Role of Rotation on the Yields of the Two γ -Ray Emitters 26 Al and 60 Fe Ejected by Massive Stars. The Astrophysical Journal. 991(1). 21–21.
3.
Allen, Mark, Peter L. Biermann, A. Chieffi, et al.. (2024). Loaded layer-cake model for cosmic ray interaction around exploding super-giant stars making black holes. Astroparticle Physics. 161. 102976–102976.
4.
Limongi, Marco, et al.. (2023). Explosion Mechanism of Core-collapse Supernovae: Role of the Si/Si–O Interface. The Astrophysical Journal. 949(1). 17–17. 31 indexed citations
5.
Ventura, P., F. Dell’Agli, D. Romano, et al.. (2021). Gas and dust from extremely metal-poor AGB stars. Archivio istituzionale della ricerca (Alma Mater Studiorum Università di Bologna). 14 indexed citations
6.
Cescutti, G., F. Matteuccí, A. Chieffi, et al.. (2021). Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo. Monthly Notices of the Royal Astronomical Society. 502(2). 2495–2507. 18 indexed citations
7.
Orlando, S., M. Miceli, F. Bocchino, et al.. (2021). Modeling the Remnants of Core-collapse Supernovae from Luminous Blue Variable stars. arXiv (Cornell University). 12 indexed citations
8.
Marassi, Stefania, et al.. (2016). Dust grains from the heart of supernovae. Springer Link (Chiba Institute of Technology). 58 indexed citations
9.
Stancliffe, Richard J., A. Chieffi, John C. Lattanzio, & Ross P. Church. (2012). Why Do Low-Mass Stars Become Red Giants?. 9 indexed citations
10.
Lugaro, Maria & A. Chieffi. (2011). Radioactivites in Low- and Intermediate-Mass Stars. Lecture notes in physics. 812. 83–152. 2 indexed citations
11.
Limongi, Marco & A. Chieffi. (2009). Presupernova evolution and explosion of massive stars: the role of mass loss during the Wolf-Rayet stage.. Memorie della Societa Astronomica Italiana. 80. 151.
12.
Voss, R., R. Diehl, D. H. Hartmann, et al.. (2009). Using population synthesis of massive stars to study theinterstellar medium near OB associations. Springer Link (Chiba Institute of Technology). 31 indexed citations
13.
Limongi, Marco & A. Chieffi. (2005). Nucleosynthesis of 60 Fe in massive stars. 10 indexed citations
14.
Limongi, Marco, A. Chieffi, & P. Bonifacio. (2003). On the Origin of HE 0107-5240, the Most Iron-deficient Star Presently Known. The Astrophysical Journal. 594(2). L123–L126. 59 indexed citations
15.
Bonifacio, P., L. Pasquini, F. Spite, et al.. (2002). The lithium content of the globular clusterNGC 6397. Springer Link (Chiba Institute of Technology). 115 indexed citations
16.
Richer, Harvey B., Brad M. S. Hansen, Marco Limongi, et al.. (2000). Isochrones and Luminosity Functions for Old White Dwarfs. The Astrophysical Journal. 529(1). 318–337. 34 indexed citations
17.
Testa, V., F. R. Ferraro, A. Chieffi, et al.. (1999). The Large Magellanic Cloud Globular Cluster NGC 1866: New Data, New Models, New Analysis. The Astronomical Journal. 118(6). 2839–2864. 29 indexed citations
18.
Castellani, V., A. Chieffi, & L. Pulone. (1991). The evolution of He-burning stars - Horizontal and asymptotic branches in Galactic globulars. The Astrophysical Journal Supplement Series. 76. 911–911. 50 indexed citations
19.
Castellani, V., A. Chieffi, & L. Pulone. (1989). Theoretical models for helium-burning stars in intermediate-metallicity globular clusters. The Astrophysical Journal. 344. 239–239. 8 indexed citations
20.
D’Antona, F., R. Gratton, & A. Chieffi. (1983). CNO self-pollution in globular clusters; a model and its possible observational tests.. Memorie della Societa Astronomica Italiana. 54. 173–198. 2 indexed citations

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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026