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| Astronomers have found a “burping” supermassive black hole is 26 million light-years from Earth in the Messier 51 galaxy (which includes the picturesque Whirlpool galaxy). They used NASA’s Chandra X-ray Observatory to spot the monster black hole, which is singled out in the X-ray view inset. Credit: X-ray: NASA/CXC/Univ of Texas/E.Schlegel et al; Optical: NASA/STScI |
KISSIMMEE, Fla. — A black hole’s epic “burp” may help solve one of the deep mysteries of the galactic core.
The dust-filled expanses of spiral galaxies like the Milky Way are bursting with star formation — the dustier the area is, the more likely it is for new stars to form there. But astronomers have found that stars rarely form in the center of a galaxy, where a supermassive black hole often rests , and researchers don’t know why. Smaller, elliptical galaxies also show little star formation.
A black hole relatively close to the Milky Way — a mere 26 million light-years from earth — has shown evidence of a huge X-ray blast outward that may have “snowplowed,” or swept away, nearby star-forming dust. [The Strangest Black Holes in the Universe ]
“This is the best example of snowplowed material I’ve ever seen,” Eric Schlegel, lead author on the new study and researcher at the University of Texas at San Antonio, said in a press conference today (Jan. 5) at the American Astronomical Society’s winter meeting today in Kissimmee, Florida. “This is clearly a way of ejecting gas from a galaxy.”
“For an analogy, astronomers often refer to black holes as ‘eating’ stars and gas,” Schlegel added in a statement . “Apparently, black holes can also burp after their meal.”
Schlegel’s team analyzed data from the orbiting Chandra X-ray Observatory to investigate the dwarf galaxy NGC 5195, which is in the process of merging with the flashier Whirlpool galaxy. The researchers observed two arcs of X-rays near the center of the dwarf galaxy, which appear to be the remnants of two huge blasts outward from the black hole . Plus, the view from an optical telescope revealed a region of cooler hydrogen gas just past the X-ray arcs, which suggests the blasts pushed dust outward.
Schlegel said that dust and gas from the galaxy’s collision with the Whirlpool galaxy could have slingshotted around the black hole, but that he finds that unlikely. More probably, the black hole actually reacted to the large additional quantities of dust pushed into its path, resulting in the “burp,” he said. The inner X-ray arc may have taken about 1 million to 3 million years to expand to its current position, and the outer one 3 million to 6 million years, officials said in the statement.
There’s much more to explore about this system, Schlegel noted. “How that reaction goes is very unclear, but I think it’s clearly something that’s worthy of study at other wavelengths,” he said at the conference, “in addition to using simulations to try to [replicate] it.”
The researchers said they suspect this type of reaction might have been much more common in the early universe, when galaxies were more densely packed together, but this “nearby” galaxy exhibiting the behavior is an exciting opportunity to see it happening up close, with less distortion. The effect can reach further out than the dramatic winds that push material away from a black hole, and it is an interesting new example of how a supermassive black hole’s activity can shape a galaxy, a process called feedback, the researchers said.
Credit: NASA/CXC/Univ of Texas/E.Schlegel et al
The scientists also found something strange along the border of the blast: Although the “burp” may have swept dust-forming gas away from the center of the galaxy, enough was pushed up together outside the outer arc to form new stars, as well.
“We think that feedback keeps galaxies from becoming too large,” co-author Marie Machacek, a researcher at the Harvard-Smithsonian Center for Astrophysics, in Massachusetts, said in the statement. “But at the same time, it can be responsible for how some stars form. This shows that black holes can create, not just destroy.”
These results have been submitted to The Astrophysical Journal.
Email Sarah Lewin at slewin@space.com or follow her @SarahExplains . Follow us @Spacedotcom , Facebook and Google+ . Original article on Space.com .
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