M. Busso

10.9k total citations · 3 hit papers
173 papers, 6.7k citations indexed

About

M. Busso is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, M. Busso has authored 173 papers receiving a total of 6.7k indexed citations (citations by other indexed papers that have themselves been cited), including 140 papers in Astronomy and Astrophysics, 51 papers in Instrumentation and 38 papers in Nuclear and High Energy Physics. Recurrent topics in M. Busso's work include Stellar, planetary, and galactic studies (112 papers), Astro and Planetary Science (88 papers) and Astronomy and Astrophysical Research (51 papers). M. Busso is often cited by papers focused on Stellar, planetary, and galactic studies (112 papers), Astro and Planetary Science (88 papers) and Astronomy and Astrophysical Research (51 papers). M. Busso collaborates with scholars based in Italy, United States and Germany. M. Busso's co-authors include R. Gallino, G. J. Wasserburg, O. Straniero, C. M. Raiteri, C. Arlandini, Maria Lugaro, Marco Limongi, Kenneth M. Nollett, C. Travaglio and S. Palmerini and has published in prestigious journals such as Nature, Proceedings of the National Academy of Sciences and The Journal of Chemical Physics.

In The Last Decade

M. Busso

154 papers receiving 6.5k citations

Hit Papers

Nucleosynthesis in Asymptotic Giant Branch Stars: Relevan... 1998 2026 2007 2016 1999 1999 1998 200 400 600

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. Busso Italy 41 5.4k 2.3k 994 501 437 173 6.7k
F. Fiore Italy 50 8.6k 1.6× 2.9k 1.3× 1.7k 1.7× 139 0.3× 33 0.1× 303 8.9k
P. R. Wood Australia 45 6.8k 1.3× 263 0.1× 2.9k 2.9× 46 0.1× 105 0.2× 241 7.6k
Brian D. Warner South Africa 27 3.4k 0.6× 409 0.2× 100 0.1× 101 0.2× 502 1.1× 286 3.8k
Stirling A. Colgate United States 31 3.6k 0.7× 2.1k 0.9× 56 0.1× 178 0.4× 249 0.6× 149 4.6k
G. R. Burbidge United States 32 4.5k 0.8× 3.2k 1.4× 847 0.9× 516 1.0× 146 0.3× 297 6.3k
William D. Cochran United States 38 4.5k 0.8× 163 0.1× 1.3k 1.3× 70 0.1× 98 0.2× 218 5.1k
F. E. Marshall United States 25 2.4k 0.4× 937 0.4× 123 0.1× 155 0.3× 289 0.7× 204 2.9k
T. Rauscher Switzerland 42 3.3k 0.6× 5.6k 2.5× 198 0.2× 1.8k 3.7× 458 1.0× 258 7.9k
R. D. Hoffman United States 24 3.2k 0.6× 2.8k 1.2× 270 0.3× 483 1.0× 239 0.5× 53 4.6k
R. Michael Rich United States 59 11.0k 2.1× 756 0.3× 5.6k 5.7× 12 0.0× 111 0.3× 339 11.4k

Countries citing papers authored by M. Busso

Since Specialization
Citations

This map shows the geographic impact of M. Busso'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 M. Busso with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Busso more than expected).

Fields of papers citing papers by M. Busso

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. Busso. 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 M. Busso. The network helps show where M. Busso may publish in the future.

Co-authorship network of co-authors of M. Busso

This figure shows the co-authorship network connecting the top 25 collaborators of M. Busso. A scholar is included among the top collaborators of M. Busso 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 M. Busso. M. Busso 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.
Palmerini, S., M. Busso, D. Vescovi, et al.. (2023). Presolar grain isotopic ratios as constraints to nuclear physics inputs for s-process calculations. SHILAP Revista de lepidopterología. 279. 6006–6006. 1 indexed citations
2.
Palmerini, S., S. Cristallo, L. Piersanti, D. Vescovi, & M. Busso. (2021). Group II Oxide Grains: How Massive Are Their AGB Star Progenitors?. Universe. 7(6). 175–175. 5 indexed citations
3.
Lebzelter, T., S. Uttenthaler, M. Busso, M. Schultheis, & B. Aringer. (2012). Lithium abundances along the red giant branch: FLAMES-GIRAFFE spectra of a large sample of low-mass bulge stars. Springer Link (Chiba Institute of Technology). 27 indexed citations
4.
Palmerini, S., M. Busso, M. La Cognata, & S. Cristallo. (2010). Effects of new reaction rates on p-capture nucleosynthesis in Low Mass Stars. 130. 1 indexed citations
5.
Magrini, L., S. Randich, M. Zoccali, et al.. (2010). Open clusters towards the Galactic centre: chemistry and dynamics. A VLT spectroscopic study of NGC 6192, NGC 6404, NGC 6583. Americanae (AECID Library). 34 indexed citations
6.
Palmerini, S., et al.. (2008). The Ninth Torino Workshop on Evolution and Nucleosynthesis in AGB Stars and The Second Perugia Workshop on Nuclear Astrophysics. AIPC. 1001. 1 indexed citations
7.
Busso, M.. (2007). Nuclear Processes in AGB Stars. ASPC. 378. 26. 1 indexed citations
8.
Uttenthaler, S., T. Lebzelter, S. Palmerini, et al.. (2007). Low-mass lithium-rich AGB stars in the Galactic bulge: evidence for\n cool bottom processing?. Springer Link (Chiba Institute of Technology). 20 indexed citations
9.
Ciprini, S., M. Busso, G. Tosti, & P. Persi. (2003). IV National Conference on Infrared Astronomy. Memorie della Societa Astronomica Italiana. 74. 1–269.
10.
Corcione, L., et al.. (2003). Control system architecture for mid-infrared cameras: from TIRCAM2 to IRAIT. MmSAI. 74. 57. 1 indexed citations
11.
Tosti, G., et al.. (2003). IRAIT: a Telescope for Infrared Astronomy from Antarctica. Memorie della Societa Astronomica Italiana. 74. 37. 1 indexed citations
12.
Nollett, Kenneth M., M. Busso, & G. J. Wasserburg. (2002). Cool Bottom Processing on the AGB and Presolar Grain Compositions. Lunar and Planetary Science Conference. 1385. 1 indexed citations
13.
Мішеніна, Т. В., V. V. Kovtyukh, C. Soubiran, C. Travaglio, & M. Busso. (2002). Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution. Springer Link (Chiba Institute of Technology). 90 indexed citations
14.
Ryan, Sean G., Wako Aoki, John E. Norris, et al.. (2001). s- and r-process elements in two very metal-poor stars. University of Hertfordshire Research Archive (University of Hertfordshire). 72. 337–346. 1 indexed citations
15.
Busso, M. & R. Gallino. (2001). Salting the early soup: trace nuclei from stars to the solar system. Memorie della Societa Astronomica Italiana. 72. 239–466. 4 indexed citations
16.
Wasserburg, G. J., R. Gallino, & M. Busso. (1998). A Test of the Supernova Trigger Hypothesis with 60Fe and 26Al. LPI. 1097. 2 indexed citations
17.
Gallino, R., M. Busso, C. Arlandini, Maria Lugaro, & O. Straniero. (1996). Neutron captures in low mass AGB stars. MmSAI. 67. 761. 2 indexed citations
18.
Zinner, E., S. Amari, C. Travaglio, et al.. (1995). The Isotopic Composition of Interstellar Graphite from the Murchison Meteorite: Evidence for Supernova Mixing. Lunar and Planetary Science Conference. 26. 1561. 3 indexed citations
19.
Busso, M., R. Gallino, C. M. Raiteri, & G. J. Wasserburg. (1994). Light Element Isotopic Composition in the Wind of a Typical AGB Star. Lunar and Planetary Science Conference. 209. 1 indexed citations
20.
Scaltriti, F., M. Busso, & A. Cellino. (1985). Some Comments on the Minima of the RS CVn Type Eclipsing Binaries CQ Aur, RU Cnc, VV Mon and SZ Psc. IBVS. 2841. 1. 1 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.

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