most citedDistinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics

72 citations · 126 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202054 cited

Stellar Masses of Giant Clumps in CANDELS and Simulated Galaxies Using Machine Learning

M. Huertas-Company, Y. Guo, O. Ginzburg +12

A significant fraction of high redshift star-forming disc galaxies are known to host giant clumps, whose nature and role in galaxy evolution are yet to be understood. In this work…

astro-ph.CO2020

Ly Blobs from Cold Streams Undergoing Kelvin-Helmholtz Instabilities

Nir Mandelker, Frank C. van den Bosch, Daisuke Nagai +3

We present an analytic toy model for the radiation produced by the interaction between the cold streams thought to feed massive halos at high redshift and their hot CGM. We begin b…

astro-ph.GA2019

Instability of Supersonic Cold Streams Feeding Galaxies IV: Survival of Radiatively Cooling Streams

Nir Mandelker, Daisuke Nagai, Han Aung +3

We study the effects of Kelvin Helmholtz Instability (KHI) on the cold streams that feed massive halos at high redshift, generalizing our earlier results to include the effects of…

astro-ph.GA2019

Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems

Nir Mandelker, Frank C. van den Bosch, Volker Springel +1

We present a new cosmological zoom-in simulation, where the zoom region consists of two halos with virial mass M_v~5x10^{12}M_{sun} and a ~Mpc long cosmic filament connecting them…

astro-ph.GA2019

Ultraviolet Perspectives on Diffuse Gas in the Largest Cosmic Structures

Joseph N. Burchett, Daisuke Nagai, Iryna Butsky +31

The past decade has seen an explosion of discoveries and new insights into the diffuse gas within galaxies, galaxy clusters, and the filaments composing the Cosmic Web. A new decad…

astro-ph.GA2019

Kelvin-Helmholtz Instability in Self-Gravitating Streams

Han Aung, Nir Mandelker, Daisuke Nagai +2

Self-gravitating gaseous filaments exist on many astrophysical scales, from sub-pc filaments in the interstellar medium to Mpc scale streams feeding galaxies from the cosmic web. T…