Effect of feedback on the escape of ionizing radiation from high-z galaxies
Authors/Creators
- 1. Institut d'Astrophysique de Paris, Centre de Recherche en Astrophysique de Lyon
- 2. Centre de Recherche en Astrophysique de Lyon
- 3. Oxford Astrophysics, Centre de Recherche en Astrophysique de Lyon
- 4. Oxford Astrophysics
Description
Quantifying how much of the ionizing radiation produced in high-redshift galaxies escapes in the IGM is one of the main challenges in understanding the sources of reionization. We investigate the radiative properties of simulated low mass galaxies (halos of a few 109 Msun at z=6), where radiation is modelled on-the-fly, and different sources of feedback (from stars and AGN) are included.
Using radiation-hydrodynamic simulations performed with Ramses-RT we study how the energy and momentum input from supernovae and black hole activity modulates the properties of the interstellar medium and therefore how, and how many, photons can escape from the galaxy.
I will present simulations showing (Trebitsch et al. 2017, https://arxiv.org/abs/1705.00941) that stellar feedback has a pivotal role in regulating the escape fraction in dwarf galaxies. Supernovae carve holes in the gas distribution, through which ionizing photons can escape.
Notes
Files
maximetrebitsch_printout.pdf
Additional details
Related works
- References
- arXiv:1705.00941 (arXiv)
Funding
- European Commission
- COSMOCOMP - Pan-European training in computational cosmology: modelling cosmic structures 238356
- European Commission
- GASAROUNDGALAXIES - Studying the gas around galaxies with the Multi Unit Spectroscopic Explorer and hydrodynamical simulations 278594
- European Commission
- BLACK - The formation and evolution of massive black holes 614199