We study the population of supermassive black holes (SMBHs) and their effects on massive
central galaxies in the IllustrisTNG cosmological hydrodynamical simulations of galaxy …

In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …

We present a novel implementation of supermassive black hole (SMBH) formation,
dynamics and accretion in the massively parallel tree+ SPH code, ChaNGa. This approach …

Spectroscopic surveys of the Milky Way's stars have revealed spatial, chemical, and
kinematical structures that encode its history. In this work, we study their origins using a …

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 correlations …

Quasar-mode Feedback in Nearby Type 1 Quasars: Ubiquitous Kiloparsec-scale Outflows and
Correlations with Black Hole Properties - IOPscience This site uses cookies. By continuing to …

We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …

We present the first results from romulusc, the highest resolution cosmological
hydrodynamic simulation of a galaxy cluster run to date. romulusc, a zoom-in simulation of a …

We present the first chemical evolution model for Enceladus, alias the Gaia Sausage, to
investigate the star formation history of one of the most massive satellites accreted by the …

We revisit the predictions for the merger rate of massive black hole binaries detectable by
the Laser Interferometer Space Antenna (LISA) and their background signal for pulsar-timing …