Stellar Population research is conducted to study the early formation history of our Milky Way galaxy and nearby satellite galaxies. Computational stellar models are compared to observations from the Hubble Space Telescope and other optical/infrared telescopes to determine the ages of stars. FACULTY CONTACT: Brian Chaboyer
[more]We are part of a team that has discovered a population of extreme starburst galaxies with star formation densities millions of times higher than in our Milky Way. These galaxies are associated with winds being launched at thousands of km/s into the intergalactic medium, and appear to represent the most extreme possible conditions for star formation in the Universe.
[more]One idea for the formation of supermassive black holes is that they grew from lower-mass "seeds" that formed in the first generation of galaxies in the early Universe. In this scenario, some such seed black holes should remain today and provide a "fossil" record of the early cosmic formation of black holes.
[more]The luminous radiation from growing supermassive black holes (known as "active galactic nuclei" or "AGN") is effective at photoionizing the gas clouds in the host galaxy, producing huge ionized nebulae (or "narrow-line regions") glowing like fluorescent lamps that are thousands of light-years across. We are investigating the physical processes that form these nebulae, by measuring their physical sizes using optical spectroscopy from the Southern African Large Telescope (SALT) and MDM Observatory. FACULTY CONTACT: Ryan Hickox
[more]In the past decade it has become increasingly clear that the cosmic evolution of galaxies is linked to the growth of their central supermassive black holes, but the nature of this connection remains poorly understood.
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