Mathematics – Logic
Scientist
Mathematics
Logic
Scientist
University of Sheffield, United Kingdom
Kavli Institute for Astronomy and Astrophysics, Peking University & The Astrophysical Journal, China
Department of Physics and Astronomy, University of Sheffield, Sheffield, UK; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing, China
University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK
Department of Physics and Astronomy, University of Sheffield, UK
University of Virginia
Instituto de Astrofísica de Andalucía
Department of Physics and Astronomy, University of Sheffield;, National Astronomical Observatoires, Chinese Academy of Sciences
Department of Physics and Astronomy, The University of Sheffield; National Astronomical Observatoires, Chinese Academy of Sciences
Kapteyn Institute, Groningen
Department of Physics and Astronomy, The University of Sheffield, Sheffield S3 7RH, UK; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, P. R. China of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Peking University, Kavli Institute for Astronomy and Astrophysics, China
Department of Physics and Astronomy, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK; and National Astronomical Observatoires, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China
Kavli Institute for Astronomy and Astrophysics, Peking University, China
Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH, UK; National Astronomical Observatoires, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, PR China
Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
University of Sheffield
Cambridge, UK
Astronomy Department, University of Virginia
D
"Super" Star Clusters
A "super" star cluster grown old: the most massive star cluster in the Local Group
A Neutron Star with a Massive Progenitor in the Star Cluster Westerlund 1
A Neutron Star with a Massive Progenitor in Westerlund 1
A New Diagnostic Method for Assessment of Stellar Stratification in Star Clusters
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