Astronomers have discovered eight new black hole binaries that echo around our galaxy, allowing them to piece together a common picture of how a black hole moves in an explosion, according to a new study.
The findings of the research were published in the 'The Astrophysical Journal' by MIT graduate student Jingyi Wang and other co-authors including Matteo Lucchini and Ron Remillard at MIT, along with collaborators from Caltech and other institutions.
Scattered across our Milky Way galaxy are tens of millions of black holes, immensely strong gravitational wells of spacetime, from which infalling matter, and even light, can never escape. Black holes are dark by definition, except on rare occasions when they feed.
As a black hole pulls in gas and dust from an orbiting star, it can give off spectacular bursts of X-ray light that bounce and echo off the inspiraling gas, briefly illuminating a black hole's extreme surroundings.
Now MIT astronomers are looking for flashes and echoes from nearby black hole X-ray binaries -- systems with a star orbiting, and occasionally being eaten away by a black hole. They are analyzing the echoes from such systems to reconstruct a black hole's immediate, extreme vicinity.
In a study appearing today in the Astrophysical Journal, the researchers report using a new automated search tool, which they've coined the "Reverberation Machine," to comb through satellite data for signs of black hole echoes.
In their search, they have discovered eight new echoing black hole binaries in our galaxy. Previously, only two such systems in the Milky Way were known to emit X-ray echoes.
In comparing the echoes across systems, the team has pieced together a general picture of how a black hole evolves during an outburst. Across all systems, they observed that a black hole first undergoes a "hard" state, whipping up a corona of high-energy photons along with a jet of relativistic particles that are launched away at close to the speed of light.
The researchers discovered that at a certain point, the black hole gives off one final, high-energy flash, before transitioning to a "soft," low-energy state.
This final flash may be a sign that a black hole's corona, the region of high-energy plasma just outside a black hole's boundary, briefly expands, ejecting a final burst of high-energy particles before disappearing entirely.
These findings could help to explain how larger, supermassive black holes at the center of a galaxy can eject particles across vastly cosmic scales to shape a galaxy's formation.
"The role of black holes in galaxy evolution is an outstanding question in modern astrophysics," says Erin Kara, assistant professor of physics at MIT. "Interestingly, these black hole binaries appear to be 'mini' supermassive black holes, and so by understanding the outbursts in these small, nearby systems, we can understand how similar outbursts in supermassive black holes affect the galaxies in which they reside."
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