Physics & Astrophysics
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I did my undergraduate and postgraduate work in Canada, obtaining a BSc in Mathematical Physics from the University of Alberta, and MSc and PhD degrees in Astrophysics from McMaster University. Subsequently I worked as a research associate in the Astronomy Department of the University of California at Berkeley; as a fibre-optics scientist at a start-up company in Edmonton, Canada; as a research associate at the Space Telescope Science Institute in Baltimore (science headquarters for the Hubble Space Telescope); and as a research associate in the Theoretical Astrophysics Group at the University of Leicester. I came to Keele in 2007.
I am part of the Astrophysics Group at Keele, and a member of the Research Institute for the Environment, Physical Sciences and Applied Mathematics (EPSAM).
Much of my current research is in the general area of stellar dynamics, with emphasis on the internal structure and long-term evolution of massive star clusters; the distribution and motions of star clusters in galaxies, and how the dark-matter content of galaxies can be constrained from this; and the structure and dynamics of dark-matter haloes.
Most recently I have become particularly intrigued by the problem of nuclear star clusters, which are now known to exist at the centres of a majority of galaxies: How do these objects relate to the supermassive black holes that are also found in the centres of most galaxies, and how do the formation and growth of these "central massive objects" influence the evolution of the galaxies around them?
My work is a mixture of theory and data modelling, and I am involved with teams carrying out large observational programmes to investigate some of the issues just mentioned, and more. Please see my personal webpage for further details.
Click here for a full bibliography.
Selected Publications
Full Publications List show
Journal Articles
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2006. The M-σ Relation for Nucleated Galaxies. The Astrophysical Journal, vol. 650(1), L37-L40. doi>
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2006. Hubble Space Telescope Proper Motions and Stellar Dynamics in the Core of the Globular Cluster 47 Tucanae. The Astrophysical Journal Supplement Series, vol. 166(1), 249-297. doi>
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2005. Resolved Massive Star Clusters in the Milky Way and Its Satellites: Brightness Profiles and a Catalog of Fundamental Parameters. The Astrophysical Journal Supplement Series, vol. 161(2), 304-360. doi>
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2005. Dynamical insight into dark matter haloes. Monthly Notices of the Royal Astronomical Society, vol. 363(4), 1057-1068. doi>
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2005. The ACS Virgo Cluster Survey. VII. Resolving the connection between globular clusters and ultracompact dwarf galaxies. ASTROPHYSICAL JOURNAL, vol. 627(1), 203-223. link>
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2004. A Hubble Space Telescope census of nuclear star clusters in late-type spiral galaxies. II. Cluster sizes and structural parameter correlations. ASTRONOMICAL JOURNAL, vol. 127(1), 105-118. link>
Other
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2005. The fundamental plane of globular clusters. HIGHLIGHTS OF ASTRONOMY, VOL 13 (vol. 13, pp. 181-182). link>
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2003. Fitting dynamical models to observations. NEW HORIZONS IN GLOBULAR CLUSTER ASTRONOMY (vol. 296, pp. 101-116). link>
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2003. HST/WFPC2 proper motions in the core of 47 Tucanae. NEW HORIZONS IN GLOBULAR CLUSTER ASTRONOMY (vol. 296, pp. 147-148). link>
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2003. Velocity dispersion in the halo of omega Centauri: No need for MOND given the present data. NEW HORIZONS IN GLOBULAR CLUSTER ASTRONOMY (vol. 296, pp. 153-154). link>
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2000. Constraints on cluster formation from old globular cluster systems. MASSIVE STELLAR CLUSTERS (vol. 211, pp. 281-287). link>
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2000. The formation history of globular clusters. 33RD ESLAB SYMPOSIUM ON STAR FORMATION FROM THE SMALL TO THE LARGE SCALE (vol. 445, pp. 77-86). link>
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1996. A model for the globular cluster luminosity function. NEW LIGHT ON GALAXY EVOLUTION (p. 418). link>
Year 1
- Physics Problem Classes (a component of all year-1 modules)
- PHY-10012 Oscillations and Waves (module leader)

