Christopher Tout

Professor of Stellar Evolution

University of Cambridge

United Kingdom

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About

Christopher Tout is a Professor of Stellar Evolution at the University of Cambridge, UK. His research spans areas such as magnetic braking in binary stars, the effects of metallicity on mass loss, and the properties of hot subdwarfs. His recent publications include studies on hydrogen-deficient binary stars and the evolution of cataclysmic variables.

Articles (18)

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2025

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2024

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2024

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2024

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2024

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2022

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2022

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2022

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2022

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2021

Collaborators (3)

Avishai Gilkis

Assistant Professor

University of Cambridge

UNITED KINGDOM

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Dominic Walton

University of Hertfordshire

UNITED KINGDOM

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Matti Dorsch

University of Potsdam

GERMANY

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Christopher Tout

Research Interests

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About

Articles (18)

Hydrogen-deficient binary stars with magnetic braking

Towards a holistic magnetic braking model – II: explaining several long-term internal- and surface-spin properties of solar-like stars and the Sun

Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers

Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer

Mass–radius relation for magnetized white dwarfs from SDSS

The Common Envelope Evolution Outcome. II. Short-orbital-period Hot Subdwarf B Binaries Reveal a Clear Picture

Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer—Application in High Mass X-Ray Binaries

Discovery of three magnetic helium-rich hot subdwarfs with SALT

Criteria for Dynamical Timescale Mass Transfer of Metal-poor Intermediate-mass Stars

Towards a holistic magnetic braking model from the evolution of cataclysmic variables to stellar spin-down – I: the spin-down of fully convective M-dwarfs

An optimal envelope ejection efficiency for merging neutron stars

Evolved cataclysmic variables as progenitors of AM CVn stars

New insights into the helium star formation channel of AM CVn systems with explanations of Gaia14aae and ZTFJ1637+49

The Common Envelope Evolution Outcome—A Case Study on Hot Subdwarf B Stars

The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes

A unified model for the evolution of cataclysmic variables

Evolution of Highly Magnetic White Dwarfs by Field Decay and Cooling: Theory and Simulations

Resolving dichotomy in compact objects through continuous gravitational waves observation

Collaborators (3)

Avishai Gilkis

Dominic Walton

Matti Dorsch

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