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20242026
most citedInvestigating the Growth of Little Red Dot Descendants at z<4 with the JWST

6 citations · 8 across the 5 of their papers we have counts for

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Showing 2024Show all

12 papers · 1 filter

astro-ph.GA2024

Growth of Massive Black-Holes in FFB Galaxies at Cosmic Dawn

Avishai Dekel, Nicholas C. Stone, Dhruba Dutta Chowdhury +4

The scenario of feedback-free starbursts (FFB), which predicts excessively bright galaxies at cosmic dawn as observed using JWST, may provide a natural setting for black hole (BH)…

astro-ph.GA2024

Effects of Cloud Geometry and Metallicity on Shattering and Coagulation of Cold Gas, and Implications for Cold Streams Penetrating Virial Shocks

Zhiyuan Yao, Nir Mandelker, S. Peng Oh +2

Theory and observations reveal that the circumgalactic medium (CGM) and the cosmic web at high redshifts are multiphase, with small clouds of cold gas embedded in a hot, diffuse me…

astro-ph.GA2024

Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon

Han Aung, Nir Mandelker, Avishai Dekel +3

We explore the evolution of cold streams from the cosmic web that feed galaxies through their shock-heated circumgalactic medium (CGM) at cosmic noon, . In addition to…

astro-ph.GA2024

What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50

Abhner P. De Almeida, Gary A. Mamon, Avishai Dekel +1

Nearby dwarf galaxies display a variety of effective radii (sizes) at a given stellar mass, suggesting different evolution scenarios according to their final "stellar" size. The TN…

astro-ph.CO2024

Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history

Sarah Libanore, Jordan Flitter, Ely D. Kovetz +2

Different star-formation models at Cosmic Dawn produce detectable signatures in the observables of upcoming 21-cm experiments. In this work, we consider the physical scenario of fe…

astro-ph.GA2024

Formation of Giant Clumps in High- Disc Galaxies by Compressive Turbulence

Nir Mandelker, Omry Ginzburg, Avishai Dekel +4

We address the formation of giant clumps in violently unstable gas-rich disc galaxies at cosmic noon. While these are commonly thought to originate from gravitational Toomre instab…