Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Queen Mary, University of London
Queen Mary College, London, England
Astronomy Unit, Queen Mary and Westfield College, Mile End Road, London E1 4NS; Observatoire de Paris, Place Jules Janssen, 92155 Meudon, France
Astronomy Unit, Queen Mary, University of London Mile End Road, London E1 4NS, UK; LESIA, UMR8109, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris, 92195 Meudon Cedex, France
Queen Mary University of London, Astronomy Unit, Mile End Road, London E1 4NS, UK ; LESIA, Observatoire de Paris, Place Jules Janssen, 92195 Meudon, France
High Altitude Observatory, Boulder, Colorado, and King's College, University of London.
Astronomy Unit, Queen Mary and Westfield College, University of London, Mile End Road, London E1 4NS, UK
Department of Mathematics, Queen Mary College, University of London
School of Mathematical Sciences, University of London, Mile End Road, London E1 4NS, UK
Queen Mary College
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK; LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France
Astronomy Unit, Queen Mary and Westfield College, Mile End Road, London E1 4NS; Observatoire de Paris, Place Jules Janssen, 92195 Meudon Cedex, France
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK LESIA, Observatoire de Paris, Place Jules Janssen, 92155 Meudon, France
Queen Mary and Westfield College, London, United Kingdom
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK ; LESIA, Observatoire de Paris, Place Jules Janssen, 92195 Meudon Cedex, France
School of Mathematical Sciences, Queen Mary and Westfield College, London, UK
Queen Mary, University of London, London, United Kingdom
Astronomy Unit, Queen Mary and Westfield College, London E1 4NS
Advanced Study Program, National Center for Atmospheric Research;, Queen Mary College, University of London
Astronomy Unit, Queen Mary, University of London, Mile
(Erratum) Limits on convective penetration from stellar cores.
2-dimensional models of rapidly rotating stars I. Uniformly rotating zero age main sequence stars
2-dimensional models of rapidly rotating stars. II. Hydrostatic and acoustic models with Ω=Ω(r,θ)
A 'fast' model of the solar convection zone
A fresh look at the seismic spectrum of HD49933: analysis of 180 days of CoRoT photometry
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