Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
School of Physics and Astronomy, University of St Andrews, Scotland
Univ of St Andrews
University of St. Andrews
Univ. of St Andrews - UK
SUPA St Andrews
U. of St. Andrews
School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS
University of Sussex, England, UK
University of St Andrews, United Kingdom
School of Physics and Astronomy, University of St Andrews, St Andrews, Fife KY16 9SS
School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS
Sussex, University, Brighton, England
School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS
School of Physics and Astronomy, University of St. Andrews, St. Andrews KY16 9SS, UK
Department of Physics and Astronomy, North Haugh, St. Andrews KY16 9SS, Scotland, UK
School of Physics and Astronomy, Univ. St Andrews, KY16 9SS, UK
Astronomy Centre, University of Sussex
School of Physics and Astronomy, University of St Andrews, St Andrews, Fife, KY16 9SS, Scotland
Univ. St Andrews, UK
School of Physics and Astronomy, University of St Andrews, St Andrews, Fife KY16 9SS, Scotland
SUPA, School of Physics and Astronomy, North Haugh, St Andrews, United Kingdom
School of Physics and Astronomy, University of St Andrews, KY16 9SS, UK
Univ. St. Andrews, United Kingdom
SUPA, United Kingdom
SUPA, School of Physics and Astronomy, North Haugh, St Andrews, UK, KY16 9SS of Physics and Astronomy, University of St Andrews, Scotland KY16 PSS, UK
SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews, KY16 9SS, UK
SUPA, School of Physics and Astronomy, University of St Andrews, Scotland, UK
SUPA, School of Physics and Astronomy, University of St. Andrews St. Andrews, Fife, KY16 9BX, UK
School of Physics and Astronomy, University of St Andrews, North Haugh, Fife KY16
A family of two-dimensional nonlinear solutions for magnetic field annihilation
A further 'degree of freedom' in the rotational evolution of stars
A Multi-Phase Suzaku Study of X-rays from tau Sco
A simple model for the saturation of coronal X-ray emission of rapidly rotating late-type stars
AB Dor: Beyond the Photosphere
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Profile ID: LFWR-SCP-P-11527