I review the influence jets and the bubbles they inflate might have on their ambient gas as
they operate through a negative jet feedback mechanism (JFM). I discuss astrophysical …

Neutrino-dominated accretion flows (NDAFs) around rotating stellar-mass black holes (BHs)
are plausible candidates for the central engines of gamma-ray bursts (GRBs). NDAFs are …

We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

I start by providing an updated summary of the penalized pixel-fitting (ppxf) method that is
used to extract the stellar and gas kinematics, as well as the stellar population of galaxies …

The inefficiency of star formation in massive elliptical galaxies is widely believed to be
caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas …

Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …

The Sloan Digital Sky Survey (SDSS) has been observing the universe using the 2.5 m
Sloan Foundation Telescope (Gunn et al. 2006) at Apache Point Observatory (APO) for over …

We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …

We use deep JWST/NIRSpec R∼ 1000 slit spectra of 113 galaxies at, selected from the
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …

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 …