On the energy transfer from low power jets to the IGM
Abstract
Recent high resolution hydrodynamic simulations of Massaglia et al. 2016 with the PLUTO code have shown that low power FRI jets form turbulent structures over scales of several kilo-parsecs. We aim to carry out two simulations of jet induced feedback, with two different jet powers. One of the primary focus of the work will be to check the growth and transport of turbulence induced by the jet, the generation of sound waves and the subsequent heating of the IGM.
- Publication:
-
Memorie della Societa Astronomica Italiana
- Pub Date:
- 2020
- Bibcode:
- 2020MmSAI..91..254C