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20112024
most citedIntroducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution

130 citations · 412 across the 24 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 16 cited

Constraints from dwarf galaxies on black hole seeding and growth models with current and future surveys

Urmila Chadayammuri, Akos Bogdan, Angelo Ricarte +1

Dwarf galaxies are promising test beds for constraining models of supermassive and intermediate-mass black holes (MBH) via their black hole occupation fraction (BHOF). Disentanglin…

astro-ph.CO2022★ 24 cited

Weak-lensing mass bias in merging galaxy clusters

Wonki Lee, Sangjun Cha, M. James Jee +6

Although weak lensing (WL) is a powerful method to estimate a galaxy cluster mass without any dynamical assumptions, a model bias can arise when the cluster density profile departs…

astro-ph.HE2022

The structure of cluster merger shocks: turbulent width and the electron heating timescale

H. R. Russell, P. E. J. Nulsen, D. Caprioli +10

We present a new 2 Ms Chandra observation of the cluster merger Abell 2146, which hosts two huge M~2 shock fronts each ~500 kpc across. For the first time, we resolve and measure t…

astro-ph.CO2022★ 6 cited

The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey

Erwin T. Lau, Akos Bogdan, Urmila Chadayammuri +3

The eROSITA Final Equatorial Depth Survey (eFEDS), with a sky area of 140 square degrees with depth equivalent to the equatorial patch of the final eROSITA all-sky survey, represen…

astro-ph.GA2022★ 3 cited

Testing galaxy feedback models with the first resolved profiles of the circumgalactic medium

Urmila Chadayammuri, Akos Bogdan, Benjamin Oppenheimer +3

The hot ( K) phase of the circumgalactic medium (CGM) contains a large fraction of baryons in galaxies. It also retains signatures of the processes that shaped the galaxies,…

astro-ph.HE2022★ 14 cited

Turbulent magnetic fields in merging clusters: A case study of Abell 2146

Urmila Chadayammuri, John ZuHone, Paul Nulsen +2

Kelvin-Helmholtz Instabilities (KHI) along contact discontinuities in galaxy clusters have been used to constrain the strength of magnetic fields in galaxy clusters, following the…