Meet the AAS Keynote Speakers: Julie Comerford

In this series of posts, we sit down with a few of the keynote speakers of the 232nd AAS meeting to learn more about them and their research. You can see a full schedule of their talks here!

Hungry, hungry galaxies

Nearly every massive galaxy has a supermassive black hole at its center. In some galaxies, like our own Milky Way, the supermassive black hole is fairly passive; in fact, the Milky Way’s black hole (Sagittarius A*) is nearly invisible, and we’ve only been able to detect it by observing its gravitational interactions with the stars and gas around it.

In other galaxies, though, the supermassive black holes are a lot harder to miss. These active galactic nuclei (AGN) can take on lots of different appearances, but they all seem to be supermassive black holes that accrete large amounts of material from the galaxy. This powers tremendously energetic jets that can outshine the entire galaxy.

AGN also play an incredibly important role in how galaxies evolve. As Professor Julie Comerford describes, the two main ways that an AGN can influence the evolution of a galaxy are through fueling and feedback. Comerford, a professor at the University of Colorado Boulder, will talk about these processes during her plenary lecture at #AAS232, “Supermassive Black Hole Fueling and Feedback in Galaxies.”

Figure 1. Dr. Julie Comerford from CU Boulder

Fueling describes how gas is accreted onto the black hole, building up its mass and powering the AGN. In particular, Comerford will discuss how fueling happens during galaxy mergers: “When you merge two galaxies together, that drives lots of gas inflows towards the center onto the black holes.” Feedback, on the other hand, describes how the black hole then produces jets or winds that can heat or even expel material in the galaxy. Both of these processes prevent the gas from forming stars, helping regulate the galaxy’s star formation; this regulation is important because we know most galaxies are not efficient at forming stars.

Comerford’s research on both fueling and feedback focuses primarily on the nearby universe, where she looks for galaxy mergers in general with and without AGN. “I really like things that are a little bizarre or unexpected, and trying to explain them,” she says. For example, she recently found one galaxy that’s had two separate feedback events (Figure 2). What caused the second outflow, nearly 100,000 years after the first one? “If you zoom out from this galaxy,” Comerford says, “then you see there’s another galaxy lurking twelve kiloparsecs away.” It turns out that interactions between the galaxies likely triggered two different accretion events, producing the two different outflows!

Figure 2. Galaxy SDSS J1354+1327. The bottom arrow points to the older outflow, and the top arrow points to the more recent outflow. (Credit: NASA/STScI/CXC)

Through observations like these (and by collaborating with theorists who make simulations), she aims to build a “fuller, more complete picture” of what’s happening in these weird galaxies: “The observations are just one snapshot in time, so the simulations can help fill in the picture.”

In some ways, Comerford’s career has also been about “filling in the picture.” She had her first exposure to research in high school and loved it. So when she started undergrad, she already had the big picture in mind. “I knew I wanted to be a professor,” Comerford says, even before she figured out what field she wanted to be a professor of. She just liked the idea of both “doing research and being at the cutting-edge, and also advising students and teaching students.”

Eventually, she filled in the rest of the picture. She knew she wanted to pursue a physics-related field, so she signed up for an astrophysics class “just to cover my bases and see what it was like.” That class hooked her on astrophysics. From there, it wasn’t until grad school that she started doing AGN research.

So what advice would she give a student who hasn’t filled in the picture yet? “Surround yourself with good people,” Comerford says. Having a support network of some kind— a supportive cohort of fellow students, or good advisors and mentors—makes all the difference, and she notes that this advice applies at all career stages!

If you’re interested in hearing more about Dr. Comerford’s work, or if you want to see cool pictures of galaxies, come check out her plenary talk at 12:20PM tomorrow on Wednesday, June 6 at #AAS232.

About Mia de los Reyes

I'm a grad student at Caltech, where I study the chemical compositions of nearby dwarf galaxies. Before coming to sunny California, I spent a year as a postgrad at the University of Cambridge, studying star formation in galaxies. Now that I've escaped to warmer climates, my hobbies include rock climbing, aerial silks, and finding free food on campus.

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  1. Astrobites at AAS 232: Day 3 and Day 4 | astrobites - […] Comerford’s talk focused on two major ways that AGN can influence their host galaxy: fueling (the SMBH accretes matter)…

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