activity
20182021
most citedOrigin of the Golden Mass of Galaxies and Black Holes

25 citations · 46 across the 3 of their papers we have counts for

collaborators

11 papers

astro-ph.GA202121 cited

Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows

Avishai Dekel, Jonathan Freundlich, Fangzhou Jiang +6

Observed rotation curves in star-forming galaxies indicate a puzzling dearth of dark matter in extended flat cores within haloes of mass at . T…

astro-ph.GA2020

Compaction-Driven Black Hole Growth

Sharon Lapiner, Avishai Dekel, Yohan Dubois

We study the interplay between galaxy evolution and central black-hole (BH) growth using the {NewHorizon} cosmological simulation. BH growth is slow when the dark-matter halo is be…

astro-ph.GA2020

Evaluating Galaxy Dynamical Masses From Kinematics and Jeans Equilibrium in Simulations

Michael Kretschmer, Avishai Dekel, Jonathan Freundlich +3

We provide prescriptions to evaluate the dynamical mass () of galaxies from kinematic measurements of stars or gas using analytic considerations and the VELA suite of…

astro-ph.GA2020

The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties

Jonathan Freundlich, Fangzhou Jiang, Avishai Dekel +6

We explore a function with two shape parameters for the dark-matter halo density profile subject to baryonic effects, which is a special case of the general Zhao family of models a…

astro-ph.GA2020

Origin of Star-Forming Rings around Massive Centres in Massive Galaxies at

Avishai Dekel, Sharon Lapiner, Omri Ginzburg +9

Using analytic modeling and simulations, we address the origin of an abundance of star-forming, clumpy, extended gas rings about massive central bodies in massive galaxies at $z \!…

astro-ph.GA2019

A mass threshold for galactic gas discs by spin flips

Avishai Dekel, Omri Ginzburg, Fangzhou Jiang +4

We predict, analytically and by simulations, that gas discs tend to survive only in haloes above a threshold mass (stellar mass )…