S04
Modeling galaxies at different scales
Communauté
Contact : jonathan.freundlich@astro.unistra.fr
Main language for discussions / Langue principale des échanges oraux : ENGLISH
Galaxy formation and evolution is a crucial laboratory for testing both our understanding of the complex physical processes involved within galaxies and the limits of the current LCDM model of structure formation. This requires models spanning from local, sub-parsec processes to large-scale cosmological environments. In this SF2A workshop, we aim to welcome presentations of results obtained using all the different techniques used to model galaxies, from non-collisional dynamics and N-body methods to hydrodynamical simulations at different scales and semi-analytical models. The goal of the workshop is notably to foster discussions on the synergies, limitations, and future directions of these models.
We particularly encourage students, postdocs, and young researchers in France or with ties to the French community to present their work. Presentations will be in English.
SOC: Christian Boily, Samuel Boissier, Paola Di Matteo, Jonathan Freundlich, Anaelle Hallé, Katarina Kraljic, Nadège Lagarde, Joseph Lewis, Joakim Rosdahl
Programme des présentations orales
| Horaire | Auteur | Titre | Abstract | Présentation (fichier) |
|---|---|---|---|---|
| 14h00 – 14h15 | Patrick Hennebelle | Explaining the Schmidt-Kennicutt relation: a multi-scale analytical model | Fichier | – |
| 14h15 – 14h30 | Brucy, Noé; Vázquez-Semadeni, Enrique; Colman, Tine; Fensch, Jérémy; Klessen, Ralf S. | Does gravity drive molecular cloud assembly? | Fichier | – |
| 14h30 – 14h45 | Pierre Dumond, Gilles Chabrier, Jérémy Fensch, Etienne Jaupart | From a mass invariant in the compressible gravoturbulent ISM to the characteristic mass of the prestellar cores | Fichier | – |
| 14h45 – 15h00 | Ferrone S.M., Di Matteo, P., Montuori, M., Ibata, R., Mastrobuono-Battisti, A., Pagnini, G., | Those who part the streams: a story of globular clusters and dark matter | Fichier | – |
| 15h00 – 15h15 | Adrian Szpilfidel | Fuzzy dark matter dynamical friction and the survival of globular clusters | Fichier | – |
| 15h15 – 15h30 | Poster flash talks | |||
| 15h30 – 16h00 | Pause | |||
| 16h00 – 16h15 | Akib, I., Hammer, F., Yang, Y | Modelling the Last Major Merger that Shaped the Milky Way | Fichier | – |
| 16h15 – 16h30 | Meagher, N. Cattaneo, A. Mamon, G. | 100 years of Hubble’s Bulges: How do bulges grow in modern high-resolution Magneto-Hydrodynamical Cosmological simulations? An insight from IllustrisTNG. | Fichier | – |
| 16h30 – 16h45 | Pacheco-Arias, J. M., Epinat, B., Amram, P., Mercier, W. | The Anatomy of Angular Momentum in Galactic Discs: Insights from TNG50 | Fichier | – |
| 16h45 – 17h00 | DEDIEU, Florian ; HALLE Anaëlle ; COMBES Françoise | Nuclear ring formation in barred galaxies with hydrodynamical simulations. | Fichier | – |
| 17h00 – 17h15 | Farcy M., Hirschmann M., Occhipinti A., Somerville R. S., Choi E., Koudmani S., Naab T., Valentino F. | The impact of AGN winds on the early evolution of massive galaxies | Fichier | – |
| 17h15 – 17h30 | Matthieu Béthermin on behalf of the SIDES team | The Simulated Infrared Dusty Extragalactic Sky (SIDES): a Semi-Empirical Simulation for Long-Wavelength Extragalactic Surveys | Fichier | – |
| 17h30 – 17h45 | M. Garnichey, S. D. Vergani | Joining RAMSES simulations and LGRB afterglow spectroscopic observations to study high-redshift galaxies | Fichier | – |