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X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
Nhut Truong, Annalisa Pillepich, Norbert Werner +6
Hot gaseous atmospheres that permeate galaxies and extend far beyond their stellar distribution, where they are commonly referred to as the circumgalactic medium (CGM), imprint imp…
Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
Yuan Li, Melanie Habouzit, Shy Genel +11
We study black hole - host galaxy correlations, and the relation between the over-massiveness (the distance from the average relation) of super-massive black holes (SMBH…
The Arepo public code release
Rainer Weinberger, Volker Springel, Rüdiger Pakmor
We introduce the public version of the cosmological magnetohydrodynamical moving-mesh simulation code Arepo. This version contains a finite-volume magnetohydrodynamics algorithm on…
The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Bryan A. Terrazas, Eric F. Bell, Annalisa Pillepich +8
Supermassive black hole feedback is thought to be responsible for the lack of star formation, or quiescence, in a significant fraction of galaxies. We explore how observable correl…
A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
Dandan Xu, Ling Zhu, Robert Grand +16
Motivated by the recently discovered kinematic "Hubble sequence" shown by the stellar orbit-circularity distribution of 260 CALIFA galaxies, we make use of a comparable galaxy samp…
High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
Mark Vogelsberger, Dylan Nelson, Annalisa Pillepich +8
The James Webb Space Telescop (JWST) promises to revolutionise our understanding of the early Universe, and contrasting its upcoming observations with predictions of the CDM mod…