Lyman alpha clouds and
Large scale structure to theory
via 
SPH cosmological simulations.
I have strong interests in Galaxy Formation and 
MHD.
PAPERS
1997 RESUME
Completed Ph.D. 1998, Supervisor - Dick BondI am am now in Seattle at the University of Washington
CLICK HERE TO GO TO MY PAGE IN SEATTLE
I am investigating the high redshift universe, linking observations of
Lyman alpha clouds and
Large scale structure to theory
via SPH cosmological simulations.
I have strong interests in Galaxy Formation and MHD.
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This is a pseudo-ray traced image of a Lyman alpha simulation.
This is 5 Mpc box containing a few Lyman Alpha cloud
producing filaments and dwarf galaxies at z ~ 3.
Higher Brightness and opacity indicate higher density. Colours indicate
temperature. Red is 4,000,000K, Blue is 10,000K and purples
represent intermediate temperatures.
Note that the cores of the knots are cool and thus blue. Through the
red hot gas around them they appear purple.
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homepage
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: More roadkill on the Information Superhighway
homepage
Department of Astronomy
homepage
email: wadsley@cita.utoronto.ca