In force date
Call year
2018
Investigator
Financial institution
Financing program
Amount granted to the IAC Consortium
20.791 €
Description
Use of the Illustris-TNG cosmological simulation to explore the mechanisms responsible for the gas depletion and star formation quenching in the cluster galaxies.
Related projects

Bipolar Nebulae
This project has three major objectives: 1) To determine the physico-chemical characteristics of bipolar planetary nebulae and symbiotic nebulae, to help understanding the origin of bipolarity and to test theoretical models, mainly models with binary central stars, aimed at explaining the observed morphology and kinematics. 2) To study the low
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