Ben Keller

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Assistant Professor

University of Memphis

United States

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About

Ben Keller is an Assistant Professor at The University of Memphis, USA. His research focuses on the study of supermassive black holes, galaxy formation, and cosmic evolution, as evidenced by his recent articles exploring topics such as the variability of supermassive black holes and the relationship between galaxy shapes and dark matter. Additionally, he examines the role of stellar evolution and feedback in galaxy evolution through a variety of astrophysical models.

Recent Grants

Grant: Close

The Critical Role of the Interstellar Medium in Galaxy Formation

Open Date: 2018-02-01

Close Date: 2020-02-01

Articles (16)

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2025

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2021

Collaborators (18)

Marta Reina-Campos

McMaster University

CANADA

Ben Keller

Research Interests

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About

Recent Grants

Articles (16)

Glimmers in the Cosmic Dawn. II. A Variability Census of Supermassive Black Holes across the Universe*

The emergence and ionizing feedback of Pop III.1 stars as progenitors for supermassive black holes

A MARVEL-ous Study of How Well Galaxy Shapes Reflect Dark Matter Halo Shapes in Cold Dark Matter Simulations

Glimmers in the Cosmic Dawn: A Census of the Youngest Supermassive Black Holes by Photometric Variability*

Bursting with Feedback: The Relationship between Feedback Model and Bursty Star Formation Histories in Dwarf Galaxies

H i discs of L* galaxies as probes of the baryonic physics of galaxy evolution

Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop

Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at z ≥ 10?

PHANGS–JWST First Results: A Statistical View on Bubble Evolution in NGC 628

Where Did the Outskirts Go? Outer Stellar Halos as a Sensitive Probe of Supernova Feedback

Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies

Empirically motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations

Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution

Momentum feedback from marginally resolved H ii regions in isolated disc galaxies

A scaling relation for the molecular cloud lifetime in Milky Way-like galaxies

Constraining the formation of NGC 1052-DF2 from its unusual globular cluster population

Collaborators (18)

Marta Reina-Campos

Paul Crowther

Richard Ellis

Thomas G Williams

Elizabeth Watkins

Sebastian Trujillo-Gomez

Charlotte Christensen

Ashley Thomas Barnes

Freeke van de Voort

Michael Tremmel

James Wadsley

Mélanie Chevance

J M Diederik Kruijssen

Ahmad A Ali

Pierluigi Monaco

Yusuke Fujimoto

Aayush Saxena

Robert Feldmann

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