Predictions for the angular dependence of gas mass flow rate and metallicity in the circumgalactic medium

Predictions for the angular dependence of gas mass flow rate and metallicity in the circumgalactic medium

We use cosmological hydrodynamical simulations to examine the physical properties of the gas in the circumgalactic media (CGM) of star-forming galaxies as a function of angular orientation. We utilize TNG50 of the IllustrisTNG project, as well as the EAGLE simulation to show that observable properti...

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Bibliographic Details
Main Authors: Péroux, Céline (Author), Nelson, Dylan (Author), van de Voort, Freeke (Author), Pillepich, Annalisa (Author), Marinacci, Federico (Author), Vogelsberger, Mark (Author), Hernquist, Lars (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2021-04-01T20:57:45Z.
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