Welcome

I am an astrophysicist working in the mission planning team for the Chandra X-ray Observatory at the Harvard-Smithsonian Center for Astrophysics. My own research speciality is the study of galaxy groups, particularly in the X-ray and radio bands, with interests in elliptical galaxies and galaxy clusters. Until recently I also worked in another field, as a software developer in the Atmospheric Measurements group, preparing for the TEMPO atmospheric pollution monitoring mission, and helping with related projects involving pollution monitoring from space. These pages focus on my astrophysics research.

Recent results

A lot of my recent work has involved the Complete Local-volume Groups Sample, a set of around 50 galaxy groups selected to allow us to explore the population of such systems in the nearby universe, examine their properties, and investigate the role of the supermassive black holes in their central galaxies in regulating the thermal balance of their halos of 10 million K gas. More details of the survey can be found on the CLoGS webpage.

Optical/NIR image (white) of the galaxy group Stephan's Quintet, overlaid with X-ray emission from the collision shock (blue), infrared emission from dust and star formation (red) and emission from cold neutral hydrogen gas (pale green) tracing past tidal interactions.
Optical/NIR image (white) of the galaxy group Stephan's Quintet, overlaid with Chandra X-ray emission (blue) tracing the famous shock ridge, JWST infrared emission (red) tracing dust and star formation, and MeerKAT neutral hydrogen emission (pale green) tracing cold neutral gas in the galaxy disks and tidal tails. Major galaxies and structures are labelled, including the star formation regions SQ-A & B

I also like to work on individual systems which are exemplars of interesting physical processes. One such system, perhaps the most famous galaxy group in the sky, is Stephan's Quintet, in which the intruder galaxy NGC 7318B has collided with a group of four other galaxies at around 1000 km/s (2.2 million miles per hour). Previous tidal interactions drew gas and stars out of the galaxies in the main group into long tidal tails and filaments still visible today. The disk of the intruder galaxy has crashed into one of these, shock-heating the cold neutral hydrogen up to about 10 million Kelvin, and accelerating electrons to relativistic velocities, producing radio continuum emission. The resulting ridge of shocked emission is shown in blue in the image above.

My colleague Kamlesh Rajpurohit collected observations of the Quintet from the MeerKAT, GMRT, VLA, and LOFAR radio observatories. With these we were able to map the cold neutral hydrogen in the galaxy disks and tidal structures, as well as using the radio continuum emission to constrain the age and dynamics of the collision shock. We now know the collision to have started 20-25 million years ago at the north end of the shock ridge, and to have finished only about 5 million years ago in the south, with the intruder galaxy moving toward us almost exactly along our line of sight. More detail can be found in our two papers: A MeerKAT View of the Neutral Atomic Gas in Stephan's Quintet and A radio continuum view of Stephan's Quintet: age, dynamics and origin of the shock.

What's new