Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Theoretical Physics, University of Oxford
Oxford University
Theoretical Physics, Oxford
Dpt.Theoret.Phys., Oxford, UK
Theoretical Physics, University of Oxford, UK
Dptm of Physics, Oxford Univ., UK
University of Oxford, Oxford, UK
Oxford University, England
Smithsonian Astrophysical Observatory, Cambridge, MA, US
Rudolf Peierls Centre for Theoretical Physics, Keble Road, Oxford OX1 3NP, UK
Oxford, University, England
Department of Physics, University of Oxford, Keble Road, Oxford OX1 3NP, UK. of Theoretical Physics, University of Oxford, 1 Keble Road, Oxford 0X1 3NP, UK.
Theoretical Physics, Keble Road, Oxford OX1 3NP, England
Department of Physics, Oxford University, 1 Keble Road, Oxford 0X1 3NP, UK.
Department of Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP, UK.
Oxford, University, England; Princeton University, NJ
Department of Theoretical Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP, UK.
Oxford Univ., United Kingdom
Rudolf Peierls Centre for Theoretical Physics, Oxford University, Keble Road, Oxford OX1 3NP, UK
Theoretical Physics, Oxford University, UK
Sub-department of Theoretical Physics, Oxford University, 1 Keble Road, Oxford 0X1 3NP, UK.
Theoretical Physics, Oxford;
University of Oxford
Dpt. Theoret. Phys., Oxford, UK
Institute for Advanced Study, Princeton, NJ
Oxford University, Oxford, England
Princeton University, New Observatory, Princeton, NJ
Oxford University, Oxford, England; California Institute of Technology, Pasadena, CA
Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford OX1 3NP, UK
Princeton University, New Observatory, Princeton, N.J.
Institute for Advanced Study, Princeton, NJ; Oxford University, Oxford, England
Princeton University, New Observatory, Pr
A Dynamical Model for the Extra-planar Gas in Spiral Galaxies
A Dynamical Model of the Inner Galaxy
A new formula for disc kinematics
A search for new members of the beta Pic, Tuc-Hor and epsilon Cha moving groups in the RAVE database
A thermally stable heating mechanism for the intracluster medium: turbulence, magnetic fields and plasma instabilities
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