This map shows the geographic impact of M. Forestini'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. Forestini with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Forestini more than expected).
This network shows the impact of papers produced by M. Forestini. 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. Forestini. The network helps show where M. Forestini may publish in the future.
Co-authorship network of co-authors of M. Forestini
This figure shows the co-authorship network connecting the top 25 collaborators of M. Forestini.
A scholar is included among the top collaborators of M. Forestini 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. Forestini. M. Forestini 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.
Palacios, A., S. Talon, C. Charbonnel, & M. Forestini. (2003). Rotational mixing in low-mass stars. Astronomy and Astrophysics. 399(2). 603–616.108 indexed citations
Lattanzio, John C., M. Forestini, & C. Charbonnel. (2000). Nucleosynthesis in intermediate mass AGB stars.. CERN Bulletin. 71. 737–744.2 indexed citations
6.
Kahane, C., Élise Dufour, M. Busso, et al.. (2000). Improved isotopic ratio determinations in IRC+10216, the progenitor mass and the s process. 357. 669–676.2 indexed citations
7.
Lattanzio, John C. & M. Forestini. (1999). Nucleosynthesis in AGB Stars. Symposium - International Astronomical Union. 191. 31–40.21 indexed citations
8.
Siess, L., M. Forestini, & C. Bertout. (1999). Physics of accretion onto young stars: III. Comparisons with observations. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 342(2). 480–491.4 indexed citations
9.
Beust, H., et al.. (1997). Dynamics and evolutionary status of the young triple stellar system, TY Coronae Austinae. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 320(2). 478–496.2 indexed citations
10.
Bouvier, J., M. Forestini, & S. Allain. (1997). The angular momentum evolution of low-mass stars. 326(3). 1023–1043.12 indexed citations
11.
Siess, L., M. Forestini, & C. Dougados. (1997). Synthetic Hertzsprung-Russell diagrams of open clusters. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 324(2). 556–565.3 indexed citations
12.
Siess, L. & M. Forestini. (1996). Physics of accretion onto young stars. I. Parametric models.. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 308(2). 472–480.
Mowlavï, N. & M. Forestini. (1994). Semi-convection and overshooting in intermediate-mass and massive stars. 282(3). 843–857.1 indexed citations
17.
Guélin, M., M. Forestini, P. Valiron, et al.. (1994). Nucleosynthesis in AGB stars: Observation of Mg-25 and Mg-26 in IRC+10216 and possible detection of Al-26. NASA Technical Reports Server (NASA). 297(1). 183–196.15 indexed citations
18.
Forestini, M.. (1994). Low-mass stars: pre-main sequence evolution and nucleosynthesis. 285(2). 473–488.3 indexed citations
19.
Forestini, M., S. Goriely, A. Jorissen, & M. Arnould. (1992). Fluorine Production in Thermal Pulses on the Asymptotic Giant Branch. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 261(1). 157–163.16 indexed citations
20.
Forestini, M., et al.. (1990). Application of an extended mixing length model to the convective envelope of the sun and its Li and Be content. 240(2). 515–519.
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
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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.