Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astronomy Unit, Queen Mary, University of London
Astronomy Unit, School of Mathematical Sciences, Queen Mary & Westfield College
Astronomy Unit, Queen Mary & Westfield College
Cambridge
University of Cambridge
QMUL
QMW College, London
Queen Mary and Westfield College
QMW, London
QMUL, London and DAMPT, Cambridge
Astronomy Unit, Queen Mary and Westfield College, London, UK
DAMTP, UK
QMW
Queen Mary and Westfield College, London
DAMTP, Cambridge
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, University of London, Mile End Road, London E1 4NS, UK
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, University of London, Mile End Road, London, UK
Astronomy Unit, Queen Mary & Westfield College, Mile End Road, London E14NS, UK
Astronomy Unit, Queen Mary & Westfield College, Mile End Rd, London E1 4NS, UK
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, Mile End Road, London E1 4NS, UK
Queen Mary College, London, England
DAMTP Cambridge UK
Queen Mary and Westfield College, London, England
School of Mathematical Science, Queen Mary and Westfield College, Mile End Road, London E1 4NS, UK Astronomy Unit, School of Mathematical Sciences, Queen Mary College
University of London
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, Mile End Road, London E1 4NS
Astronomy Unit, School of Mathematical Sciences, Queen Mary & Westfield College, Mile End Road, London E1 4NS
Isaac Newton Institute for Mathematical Sciences, 20 Clarkson Road, Cambridge CB3 0EH
Astronomy Unit, Queen Mary & Westfield College, University of London, Mile End Road, E14NS London, UK of Applied Math
0n the dynamics of warped accretion disks
3D-MHD simulations of an accretion disk with star-disk boundary layer
A comparison of one and two dimensional models of transonic accretion discs around collapsed objects
A Method for Calculations of Nonlinear Shear Flow: Application to Formation of Giant Planets in the Solar Nebula
A planet on an inclined orbit as an explanation of the warp in the Beta Pictoris disk
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