Rationale
- Study the impact of black hole maintenance-mode/radio-mode feedback on molecular gas inflows in massive galaxies.
- Focus on a small sample of Massive galaxies lying in cooling flow cluster (6 BCGs)
Methods
- JWST/MIRI imager (total H2, dust, SFR in the filaments) – High resolution data
- JWST/MRS spectroscopy of the central region (detailed excitation and dynamics) – High resolution data
- Photo-ionisation and shocks / Numerical hydrodynamics simulations
JWST GO 5918
https://www.stsci.edu/jwst/science-execution/program-information?id=501
References
Salomé et al., 2024, jwst.prop.5018S
Partners
French Support
