FR0 radio galaxies and their place in the radio morphology classification

D Garofalo, CB Singh - The Astrophysical Journal, 2019 - iopscience.iop.org
So-called FR0 radio galaxies have recently emerged as a family of active galaxies with all
the same properties as FRI radio galaxies except for their ratio of core to total emission …

A unified framework for X-shaped radio galaxies

D Garofalo, R Joshi, X Yang, CB Singh… - The Astrophysical …, 2020 - iopscience.iop.org
We propose a radically different picture for X-shaped radio galaxies compared with existing
models as transition objects between cold-mode accreting, low-spinning retrograde black …

Lense–Thirring effect on accretion flow from counter-rotating tori

D Pugliese, Z Stuchlik - Monthly Notices of the Royal …, 2022 - academic.oup.com
We study the accretion flow from a counter-rotating torus orbiting a central Kerr black hole
(BH). We characterize the flow properties at the turning point of the accreting matter flow …

The black hole-star formation connection over cosmic time

CB Singh, N Kulasiri, M North… - Publications of the …, 2021 - iopscience.iop.org
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 …

Inter-disks inversion surfaces

D Pugliese, Z Stuchlík - The European Physical Journal C, 2024 - Springer
We consider a counter-rotating torus orbiting a central Kerr black hole (BH) with
dimensionless spin a, and its accretion flow into the BH, in an agglomerate of an outer …

The Sub-Eddington Boundary for the Quasar Mass–Luminosity Plane: A Theoretical Perspective

D Garofalo, DJ Christian, AM Jones - Universe, 2019 - mdpi.com
By exploring more than sixty thousand quasars from the Sloan Digital Sky Survey Data
Release 5, Steinhardt & Elvis discovered a sub-Eddington boundary and a redshift …

The distribution and lifetime of powerful radio galaxies as a function of environment and redshift

D Garofalo, CB Singh, A Zack - Scientific Reports, 2018 - nature.com
Correlations between jet power and active time for z< 0.1 high excitation and low excitation
radio galaxies are explored as well as evidence in favor of a specific, non-random …

Peculiar black hole accretion rates in AGN with highest star formation rates in the universe

D Garofalo, E Pouliasis - … of the Astronomical Society of the …, 2022 - iopscience.iop.org
Pouliasis et al. explored star formation rates, black hole accretion rates, and stellar mass of
active galaxies at redshift above 3.5, uncovering a leveling off of the star formation rate at …

The unusual active galaxy H1821+ 643 and the elusive nature of FRI quasars

D Garofalo, CB Singh - … of the Astronomical Society of the Pacific, 2022 - iopscience.iop.org
The moderate spin estimate for the black hole at the center of the cool core cluster H1821+
643 motivates the completion of a story about this object's origin and evolution that was in …

Spin of the M87 black hole

D Garofalo - Annalen der Physik, 2020 - Wiley Online Library
Spin measurement of the 6.5 billion solar mass black hole in M87 from the Event Horizon
Telescope image is the latest in a series that span a wide range in values, but that tend to …