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Introduction Observatories Publications


INTRODUCTION:

Press Release at the CGPS site
Most research astronomers fall into 2 categories: theorists and observers. I fall into the latter category and spend my time designing experiments that use telescopes to test ideas, mainly about the structure of galaxies. Currently I am focusing on the behaviour of the gas between stars in our Milky Way Galaxy.

For example, I lead a team studying a mushroom-shaped cloud, GW1.23.4-1.5, bursting out of the disk of our Galaxy with the power of about 20 times that of our sun. One of the mysteries of our Milky Way is "why does it have a hot gas halo?" We wonder if clouds like GW123.4-1.5 can transport hot gas, known to surround both young and dying stars in the disk of the Galaxy, from the disk (i.e. plane) into the halo.



Radio paper on NGC 3256I also like to study the gas in galaxies that are interacting with each other and merging together. This example of a merger is NGC 3256. The red regions map neutral hydrogen gas, the blue map ionized hydrogen gas, and the green and yellow areas map the regions with stars.

OBSERVATORIES:

The data that I use in my research come most frequently from these telescopes and projects.

Canadian Galactic Plane Survey:

Hubble Space Telescope:

Australian Telescopes:


PUBLICATIONS:

Publications are listed on my CV page.