Public Release: 

UTSA-led team finds black hole affecting galactic climate

Researchers used NASA's Chandra X-Ray Observatory, launched and deployed in 1999 by Space Shuttle Columbia

University of Texas at San Antonio

IMAGE

IMAGE: Spiral galaxy NGC 5195 and the X-ray arcs Schlegel's team identified. view more

Credit: Eric Schlegel, the University of Texas at San Antonio

(San Antonio, Jan. 6, 2016) -- A team of researchers led by Eric Schlegel, Vaughn Family Endowed Professor in Physics at The University of Texas at San Antonio (UTSA), has discovered a powerful galactic blast produced by a giant black hole about 26 million light years from Earth. The black hole is the nearest supermassive black hole to Earth that is currently undergoing such violent outbursts.

Schlegel's team used NASA's Earth-orbiting Chandra X-ray Observatory to find the black hole blast in the famous Messier 51 system of galaxies. The system contains a large spiral galaxy, NGC 5194, colliding with a smaller companion galaxy, NGC 5195.

"Just as powerful storms here on Earth impact their environments, so too do the ones we see out in space," Schlegel said. "This black hole is blasting hot gas and particles into its surroundings that must play an important role in the evolution of the galaxy."

Schlegel and his colleagues detected two X-ray emission arcs close to the center of NGC 5195, where the supermassive black hole is located.

"We think these arcs represent artifacts from two enormous gusts when the black hole expelled material outward into the galaxy," said co-author Christine Jones, astrophysicist and lecturer at the Harvard-Smithsonian Center for Astrophysics (CfA). "We think this activity has had a big effect on the galactic landscape."

Just beyond the outer arc, the researchers detected a slender region of hydrogen gas emission, suggesting that X-ray emitting gas displaced the hydrogen gas from the center of the galaxy.

Moreover, the properties of the gas around the arcs suggest that the outer arc has swept up enough material to trigger the formation of new stars. This type of phenomenon, where a black hole affects its host galaxy, is called "feedback."

"We think that feedback keeps galaxies from becoming too large," said co-author Marie Machacek, astrophysicist at CfA. "But at the same time, it can be responsible for how some stars form, showing that black holes can be creative, not just destructive."

The astronomers believe the black hole's outbursts may have been triggered by the interaction of NGC 5195 with its larger companion, NGC 5194, causing gas to be funneled toward the black hole. The team estimates that it took about one to three million years for the inner arc to reach its current position, and three to six million years for the outer arc.

"The black hole's behavior may be a local example of events that commonly took place when the universe was much younger. That makes this observation potentially very important," Schlegel said.

The researchers presented their findings today at the 227th meeting of the American Astronomical Society meeting in Kissimmee, Fla. They have also described their work in a paper submitted to The Astrophysical Journal.

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NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

UTSA physics alumna Laura Vega '14 contributed to the research. She is currently a graduate student in the Fisk-Vanderbilt University physics program.

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