Parties d'ouvrages collectifs (1)
  1. 1. Arnould, M., & Goriely, S. (2012). The r-process of nucleosynthesis: The puzzle is still with us. In I. Küçük (Ed.), The r-process of nucleosynthesis: The puzzle is still with us (pp. 61-88). Croatia: InTech - Open Access Publisher.
    2.   Articles dans des revues avec comité de lecture (66)
  2. 1. Tsiatsiou, S., Meynet, G., Farrell, E., Hirai, Y., Choplin, A., Sibony, Y., Martinet, S., Guerço, R., Smith, V., Cunha, K., Goriely, S., Arnould, M., Fernandez-Trincado, J. G., & Ekström, S. (2025). Fluorine production in He-burning regions of massive stars during cosmic history. Astronomy & astrophysics, 696, 241. doi:10.1051/0004-6361/202453209
  3. 2. Arnould, M., & Goriely, S. (2020). Astronuclear Physics: A tale of the atomic nuclei in the skies. Progress in particle and nuclear physics., 103766. doi:10.1016/j.ppnp.2020.103766
  4. 3. Xu, Y., Takahashi, K., Goriely, S., Arnould, M., Ohta, M., & Utsunomiya, H. (2013). NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number A < 16. Nuclear Physics A, 918, 61.
  5. 4. Xu, Y., Goriely, S., Jorissen, A., Chen, G., & Arnould, M. (2013). Databases and tools for nuclear astrophysics applications: BRUSsels Nuclear LIBrary (BRUSLIB), Nuclear Astrophysics Compilation of REactions II (NACRE II) and Nuclear NETwork GENerator (NETGEN). Astronomy & astrophysics, 549, A106, 10. doi:10.1051/0004-6361/201220537
  6. 5. Xu, Y., Goriely, S., Arnould, M., & Takahashi, K. (2011). NACRE II: An update of the NACRE compilation of Atarget<16 charged-particle thermonuclear reaction rates for astrophysics. AIP Conference Proceedings, 1377, 463-465. doi:10.1063/1.3628446
  7. 6. Arnould, M. (2010). The evolution of massive stars and the concomitant non-explosive and explosive nucleosynthesis. Astrophysics and Space Science Proceedings,(202579), 278-343. doi:10.1007/978-3-642-10352-0_6
  8. 7. Arnould, M. (2008). The nuclear physics input to astrophysics modelling, and the R- and P-processes: Where do we stand 50 years after B2FH and cameron? EAS publications series, 32, 1-59. doi:10.1051/eas:0832001
  9. 8. Siess, L., & Arnould, M. (2008). Production of 26Al by super-AGB stars. Astronomy & astrophysics, 489(1), 395-402.
  10. 9. Binns, R. W., Wiedenbeck, M. E., Arnould, M., Cummings, A. C., de Nolfo, G. A., Goriely, S., Israel, M. H., Leske, R. A., Mewaldt, R. A., Stone, E., & Von Rosenvinge, T. (2008). The OB association origin of galactic cosmic rays. New astronomy reviews, 52, 427-430. doi:10.1016/j.newar.2008.05.008
  11. 10. Binns, R. W., Wiedenbeck, M. E., Arnould, M., Cummings, A. C., de Nolfo, G. A., Goriely, S., Israel, M. H., Leske, R. A., Mewaldt, R. A., Meynet, G., Scott, L., Stone, E., & Von Rosenvinge, T. (2007). OB associations, Wolf-Rayet stars, and the origin of galactic cosmic rays. Space Science Reviews, 130(1-4), 439-449.
  12. 11. Arnould, M., Goriely, S., & Takahashi, K. (2007). The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries. Physics Reports, 450(4-6), 97-213.
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