activity
19952010
most citedSPH simulations of tidally unstable accretion disks in cataclysmic variables

158 citations · 935 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2010★ 36 cited

SPH simulations of irradiation-driven warped accretion discs and the long periods in X-ray binaries

Stephen B. Foulkes, Carole A. Haswell, James R. Murray

We present three dimensional smoothed particle hydrodynamics (SPH) calculations of irradiation-driven warping of accretion discs. Initially unwarped planar discs are unstable to th…

astro-ph2008★ 76 cited

Populating the Galaxy with pulsars I: stellar & binary evolution

Paul Kiel, Jarrod Hurley, Matthew Bailes +1

The computation of theoretical pulsar populations has been a major component of pulsar studies since the 1970s. However, the majority of pulsar population synthesis has only regard…

astro-ph2007

Furnishing the Galaxy with Pulsars

Paul Kiel, Jarrod Hurley, Matthew Bailes +1

The majority of pulsar population synthesis studies performed to date have focused on isolated pulsar evolution. Those that have incorporated pulsar evolution within binary systems…

astro-ph2007★ 59 cited

Comprehensive simulations of superhumps

Amanda J. Smith, Carole A. Haswell, James R. Murray +2

(Abridged) We use 3D SPH calculations with higher resolution, as well as with more realistic viscosity and sound-speed prescriptions than previous work to examine the eccentric ins…

astro-ph2006★ 38 cited

Three dimensional SPH simulations of radiation-driven warped accretion discs

Stephen B. Foulkes, Carole A. Haswell, James R. Murray

We present three dimensional smoothed particle hydrodynamics (SPH) calculations of warped accretion discs in X-ray binary systems. Geometrically thin, optically thick accretion dis…

astro-ph2005★ 88 cited

Dust distribution in protoplanetary disks - Vertical settling and radial migration

Laure Barrière-Fouchet, Jean-François Gonzalez, James R. Murray +2

We present the results of a three dimensional, locally isothermal, non-self-gravitating SPH code which models protoplanetary disks with two fluids: gas and dust. We ran simulations…