Sarah Wellons

Assistant Professor

Wesleyan University

United States

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About

Sarah Wellons is an Assistant Professor at Wesleyan University in the United States. Her research focuses on astrophysical phenomena, particularly in the areas of black hole physics, active galactic nuclei feedback, and stellar feedback within the context of cosmological simulations. Recent articles authored by her cover topics such as dark matter profiles, quasar winds, and the correlation of far-infrared and radio emissions in galaxies.

Articles (14)

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2025

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2023

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2023

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2021

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2021

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2020

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2020

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2020

Collaborators (5)

Jonathan Stern

ISRAEL

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Andrew Wetzel

Associate Professor

University of California, Davis

UNITED STATES

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Jorge Moreno

Pomona College

UNITED STATES

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Sophie Koudmani

University of Hertfordshire

UNITED KINGDOM

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Robert Feldmann

Associate Professor

University of Zurich

SWITZERLAND

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Sarah Wellons

Research Interests

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About

Articles (14)

Diverse dark matter profiles in fire dwarfs: black holes, cosmic rays and the cusp–core enigma

Hooks, Lines, and Sinkers: How Active Galactic Nucleus Feedback and Cosmic-Ray Transport Shape the Far-infrared–Radio Correlation of Galaxies

Dense stellar clump formation driven by strong quasar winds in the FIRE cosmological hydrodynamic simulations

Effects of Multichannel Active Galactic Nuclei Feedback in FIRE Cosmological Simulations of Massive Galaxies

The impact of AGN-driven winds on physical and observable galaxy sizes

Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations

Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations

Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales

Running late: testing delayed supermassive black hole growth models against the quasar luminosity function

Why do black holes trace bulges (& central surface densities), instead of galaxies as a whole?

Which AGN jets quench star formation in massive galaxies?

Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations

Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies

Pressure balance in the multiphase ISM of cosmologically simulated disc galaxies

Collaborators (5)

Jonathan Stern

Andrew Wetzel

Jorge Moreno

Sophie Koudmani

Robert Feldmann

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