Communications publiées lors de congrès ou colloques nationaux et internationaux (60)
23.
De Smedt, K., Van Winckel, H., Kamath, D., Karakas, A. I., Siess, L., Goriely, S., & Wood, P. R. (2015). Post-AGB Stars in the Magellanic Clouds as Tracers of the s-Process Nucleosynthesis. In Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time: Vol. 497 (p. 241) ASP Conference Series.24.
Doherty, C., Gil-Pons, P., Lugaro, M., Lau, H. H. B., Lattanzio, J., Siess, L., Campbell, S. S., & Petermann, I. (2015). Nucleosynthesis in Super-AGB Stars. In Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time: Vol. 497 (p. 247) ASP Conference Series.27.
Neyskens, P., Van Eck, S., Plez, B., Goriely, S., Siess, L., & Jorissen, A. (2014). Technetium Abundances in S-type AGB Stars to Constrain Mixing and Nucleosynthesis Processes. The Tenth Pacific Rim Conference on Stellar Astrophysics. Vol. 482 (p. 81).28.
Doherty, C., Lugaro, M., Lau, H., Siess, L., Lattanzio, J., & Gil-Pons, P. (2012). Production of Short-Lived Radioactive Nuclei in Super Asymptotic Giant Branch Star. Meteoritics and Planetary Science Supplement (p. id.5159) 75th Annual Meeting of the Meteoritical Society(August 12-17, 2012: Cairns, Australia).33.
Neyskens, P., Van Eck, S., Plez, B., Goriely, S., Siess, L., & Jorissen, A. (2011). Abundance Patterns in S-type AGB Stars: Setting Constraints on Nucleosynthesis and Stellar Evolution Models. Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Vol. 445 (p. 77).