activity
20172023
most citedStrength of the Solar Coronal Magnetic field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-light Observations

41 citations · 153 across the 13 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2023★ 2 cited

Zooming in on the circumgalactic medium: resolving small-scale gas structure with the GIBLE cosmological simulations

Rahul Ramesh, Dylan Nelson

We introduce Project GIBLE (Gas Is Better resoLved around galaxiEs), a suite of cosmological zoom-in simulations where gas in the circumgalactic medium (CGM) is preferentially simu…

astro-ph.GA2023★ 3 cited

Azimuthal Anisotropy of Magnetic Fields in the Circumgalactic Medium Driven by Galactic Feedback Processes

Rahul Ramesh, Dylan Nelson, Volker Heesen +1

We use the TNG50 cosmological magnetohydrodynamical simulation of the IllustrisTNG project to show that magnetic fields in the circumgalactic medium (CGM) have significant angular…

astro-ph.GA2023★ 9 cited

Milky Way and Andromeda analogs from the TNG50 simulation

Annalisa Pillepich, Diego Sotillo-Ramos, Rahul Ramesh +7

We present the properties of Milky Way- and Andromeda-like (MW/M31-like) galaxies simulated within TNG50, the highest-resolution run of the IllustrisTNG suite of CDM magneto-hyd…

astro-ph.GA2023★ 36 cited

The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs

Rahul Ramesh, Dylan Nelson, Annalisa Pillepich

We use the TNG50 simulation of the IllustrisTNG project to study cold, dense clouds of gas in the circumgalactic media (CGM) of Milky Way-like galaxies. We find that their CGM is t…

astro-ph.GA2023★ 15 cited

The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies

Alina Boecker, Nadine Neumayer, Annalisa Pillepich +4

We investigate the origin of stars in the innermost of galaxies spanning stellar masses of at using the cos…