Britton Smith

Reader

University of Edinburgh

United Kingdom

Research Interests

Explore related searches

Professors in United Kingdom Professors in Astronomy Astronomy professors in United Kingdom

Contact this professor

Get a free first email built on one of their papers, ready for you to edit and send yourself.

About

Britton Smith is a Reader at the University of Edinburgh in the United Kingdom. His research focuses on the impacts of the metagalactic ultraviolet background on circumgalactic medium absorption systems, as well as the evolution of angular momentum in Milky Way-like galaxies. Recent contributions also include studies on super-Eddington accretion conditions and analyzing star formation feedback mechanisms in cosmological simulations.

Articles (10)

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2024

Year:

2024

Year:

2024

Year:

2022

Year:

2022

Year:

2021

Collaborators (6)

Devin W. Silvia

Michigan State University

UNITED STATES

View details

Brian O'Shea

Professor

Michigan State University

UNITED STATES

View details

Jose Oñorbe

Universidad de Sevilla

SPAIN

View details

Ayan Acharyya

Johns Hopkins University

UNITED STATES

View details

John Wise

Professor

Georgia Institute of Technology

UNITED STATES

View details

Desika Narayanan

Assistant Professor

University of Florida

UNITED STATES

View details

ApplyKite TwinLearns as you apply

Make your next move.

Prepare your application

Review drafts before you send them.

Britton Smith

Research Interests

Explore related searches

Contact this professor

About

Articles (10)

Figuring Out Gas and Galaxies in Enzo (FOGGIE). IX. The Angular Momentum Evolution of Milky Way–like Galaxies and Their Circumgalactic Gas

Figuring Out Gas and Galaxies In Enzo (FOGGIE). VIII. Complex and Stochastic Metallicity Gradients at z > 2

Impacts of the Metagalactic Ultraviolet Background on Circumgalactic Medium Absorption Systems

Conditions for super-Eddington accretion onto the first black holes

Figuring Out Gas and Galaxies in Enzo (FOGGIE). VII. The (Dis)assembly of Stellar Halos

simba-EoR: early galaxy formation in the simba simulation including a new sub-grid interstellar medium model

Why does the Milky Way have a metallicity floor?

Analyzing Star Formation Feedback Mechanisms in Cosmological Simulations

The Cosmic Mach Number as an environment measure for the underlying dark matter density field

Figuring Out Gas & Galaxies In Enzo (FOGGIE). V. The Virial Temperature Does Not Describe Gas in a Virialized Galaxy Halo

Collaborators (6)

Devin W. Silvia

Brian O'Shea

Jose Oñorbe

Ayan Acharyya

John Wise

Desika Narayanan

Make your next move.