Ouvrages publiés à titre de seul auteur (1)

  1. 1. Jorissen, A. (2021). Symphonie pour un nouveau monde,: au-delà de la dualité esprit-matière. Louvain-la-Neuve: Académia.
  2.   Ouvrages publiés en collaboration (1)

  3. 1. Sterken, C., Manfroid, J., Beele, D., de Koff, S., Eggenkamp, I., Gocking, K., Jorissen, A., Kaufer, A., Kuss, C., Schoenmakers, A., Stil, J., van Loon, J., Vink, J., Vrielmann, S., & Walde, E. (1995). Fourth Catalogue of Stars Measured in the Long-Term Photometry of Variables Project (1992 - 1994). Garching bei München: European Southern Observatory.
  4.   Ouvrages édités à titre de seul éditeur ou en collaboration (1)

  5. 1. Jorissen, A., Goriely, S., Siess, L., Rayet, M., & Boffin, H. (2004). The Future Astronuclear Physics: From Microscopic Puzzles to Macroscopic Nightmares. Paris: EDP sciences.
  6.   Parties d'ouvrages collectifs (3)

  7. 1. Jorissen, A., Van Eck, S., & Boffin, H. (2016). Velocity Fields in Stellar Atmospheres Probed by Tomography. In H. Boffin, G. Hussain, & L. Schmidtobreick (Eds.), Astronomy at High Angular Resolution - A Compendium of Techniques in the Visible and Near-Infrared (1 ed., pp. 137-154). Switzerland: Springer.(Astrophysics and Space Science Library, 439). doi:10.1007/978-3-319-39739-9
  8. 2. Jorissen, A., & Frankowski, A. (2008). Detection methods for binaries involving low- and intermediate-mass stars. In P. Pellegrini (Ed.), Graduate School in Astronomy: XII Special Courses at the National Observatory of Rio de Janeiro (pp. 3-55). American Institute of Physics.(AIP conference proceedings, 1057). doi:10.1063/1.2999998
  9. 3. Jorissen, A. (2004). AGB stars in binaries and their progeny. In H. J. Habing & H. Olofsson (Eds.), Asymptotic Giant Branch Stars (pp. 461-518). New York: Springer Verlag.(A&A Library).
  10.   Articles dans des revues avec comité de lecture (228)

  11. 1. Vanden Broeck, G., Merle, T., Mai, N. T., Van Eck, S., Goriely, S., Siess, L., Jorissen, A., & Hoai, D. T. (2026). The chemical fingerprint of the Gaia BH3 system. Evidence for early cluster enrichment from the analysis of 51 elements. Astronomy and Astrophysics Letters.
  12. 2. Merle, T., Jorissen, A., Alexandre, S., Desuter, J., Loup, C., Tokovinin, A. A., Traven, G., Van Der Swaelmen, M., Van Eck, S., Van De Steene, G., Southworth, J., & Sadowski, G. (2026). The SB9 catalogue: status, comparison with non-single stars from Gaia DR3, and evolution to SBX. Monthly notices of the Royal Astronomical Society, 547(2), 28. doi:10.1093/mnras/stag351
  13. 3. Drevon, J., Paladini, C., Höfner, S., Planquart, L., Siess, L., Jorissen, A., Montargès, M., Vlemmings, W. H., Khouri, T., Olofsson, H., Alonso-Hernandez, J., De Beck, E., Fonfria, J. P., Hron, J., Matter, A., Nardetto, N., Ohnaka, K., Sanchez-Contreras, C., Weigelt, G., Wittkowski, M., Bojnordi Arbab, B., Aringer, B., Baron, F., Chiavassa, A., Cruzalèbes, P., Danchi, W. C., Kerschbaum, F., Leftley, J., Lagadec, E., Lopez, B., Lykou, F., Millour, F., Rau, G., Sanchez Bermudez, J., Thévenin, F., Van Eck, S., & Velilla-Prieto, L. (2026). Direct imaging of mass transfer and circumcompanion structures in pi1 Gru with VLTI/MATISSE. Astronomy & astrophysics, 706, L1. doi:10.1051/0004-6361/202558298
  14. 4. Riyas, A., Karinkuzhi, D., Van Eck, S., Choplin, A., Goriely, S., Siess, L., Keerthy, M., Jorissen, A., & Merle, T. (2026). Abundance of heavy r-process elements in CEMP-rs stars: The role of the i-process. Astrophysical Journal, 997, 44.
  15. 5. Shetye, S., Van Eck, S., Jorissen, A., Escorza Santos, A., Siess, L., Goriely, S., Van Winckel, H., Uttenthaler, S., & Wijsen, N. (2025). Technetium-rich M stars: Prime diagnostics of recent third dredge-up events on the asymptotic giant branch. Astronomy & astrophysics, 702, 39.
  16. 6. Shetye, S., Van Eck, S., Jorissen, A., Escorza, A., Siess, L., Goriely, S., Van Winckel, H., Uttenthaler, S., & Wijsen, N. (2025). Technetium-rich M stars: Prime diagnostics of recent third dredge-up events on the asymptotic giant branch. Astronomy & astrophysics, 702, A39. doi:10.1051/0004-6361/202555581

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