activity
20192026
most citedA unified framework for X-shaped radio galaxies

22 citations · 38 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Winds Versus Jets in Active Galactic Nuclei

David Garofalo, Chandra B. Singh, Atticus Magerko +3

The well-established anti-correlation between disk winds and relativistic jets in X-ray binaries is often interpreted in a scale-invariant black hole accretion context. If so, acti…

astro-ph.GA2025

Why Jet Power and Star Formation Are Uncorrelated in Active Galaxies

David Garofalo, Brent McDaniel, Max North

Jet luminosity from active galaxies and the rate of star formation have recently been found to be uncorrelated observationally. We show how to understand this in the context of a m…

astro-ph.GA2023★ 4 cited

M- relations across space and time

David Garofalo, Damian J. Christian, Chase Hames +4

Feedback from active galactic nuclei (AGN) has long been invoked to explain the correlation between black hole mass and stellar velocity dispersion (M-) discovered in low redshi…

astro-ph.HE2021

The black hole-star formation connection over cosmic time

Chandra B. Singh, Nelitha Kulasiri, Max North +1

Observations at low redshift have begun to tease out the star formation rate in active galaxies (AGN), which marks the beginning of the black hole-star formation connection over co…

astro-ph.HE2020★ 12 cited

Why radio quiet quasars are preferred over radio loud quasars regardless of environment and redshift

David Garofalo, Max North, Leanne Belga +1

Evidence has accumulated suggesting the clustering of radio loud quasars is greater than for radio quiet quasars. We interpret these results in a context in which the fraction of r…

astro-ph.HE2019★ 22 cited

A unified framework for X-shaped radio galaxies

David Garofalo, Ravi Joshi, Xiaolong Yang +3

We propose a radically different picture for X-shaped radio galaxies compared to existing models as transition objects between cold mode accreting low spinning retrograde black hol…