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19952026
most citedEvolution of binary stars and the effect of tides on binary populations

2k citations · 12k across the 139 of their papers we have counts for

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Showing 2018Show all

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astro-ph.SR2018

The Magnetic Fields of White Dwarfs in Cataclysmic Variables

Gordon Briggs, Lilia Ferrario, Christopher Tout +1

The origin of magnetic fields in isolated and binary white dwarfs has been investigated in a series of recent papers. One proposal is that magnetic fields are generated through an…

astro-ph.SR2018

Origin of magnetic fields in cataclysmic variables

Gordon P. Briggs, Lilia Ferrario, Christopher A. Tout +1

In a series of recent papers, it has been proposed that high field magnetic white dwarfs are the result of close binary interaction and merging. Population synthesis calculations h…

astro-ph.GA2018★ 22 cited

The Cosmic Microwave Background and the Stellar Initial Mass Function

Adam S. Jermyn, Charles L. Steinhardt, Christopher A. Tout

We argue that an increased temperature in star-forming clouds alters the stellar initial mass function to be more bottom-light than in the Milky Way. At redshifts , he…

astro-ph.SR2018★ 82 cited

Extending Common Envelope Simulations from Roche Lobe Overflow to the Nebular Phase

Thomas A. Reichardt, Orsola De Marco, Roberto Iaconi +2

We have simulated a common envelope interaction of a 0.88-M, 90-R, red giant branch star and a 0.6-M, compact companion with the smoothed particle hyd…

astro-ph.SR2018★ 6 cited

Post-common envelope binary systems experiencing helium-shell driven stable mass transfer

Ghina M. Halabi, Robert G. Izzard, Christopher A. Tout

We evolve stellar models to study the common envelope (CE) interaction of an early asymptotic giant branch star of initial mass with a companion star of mass ran…

astro-ph.SR2018★ 25 cited

Tidal Interactions in Post Common-Envelope sdB Binaries

Holly P. Preece, Christopher A. Tout, C. Simon Jeffery

Over half of all observed hot subdwarf B (sdB) stars are found in binaries, and over half of these are found in close configurations with orbital periods of 10 or less.…