MEXICO: In a study published in the journal Nature this week, a researcher shows a link between the X-ray wind created by a supermassive black hole in the center of a galaxy and the broader dispersal of raw material that could have formed stars. A new NASA video (below) provides an easy-to-understand visualization of the process.
Using the Herschel Space Observatory and the X-ray Imaging Spectrometer attached to the Suzaku astronomy satellite, the researchers looked at galaxy F11119+3257, located an extremely far 2.3 billion light-years away. At the center of that galaxy is a black hole as massive as 16 million of our suns.
“Scientists think ultraluminous infrared galaxies like F11119 represent an early phase in the evolution of quasars, a type of black-hole-powered galaxy with extreme luminosity across a broad wavelength range,” NASA says in a report about the research.
Emanating from the center of the black hole, the researchers found gas racing outward at a speed of 170 million mph, creating what’s known as an X-ray wind. The wind arises because the voracious black hole is devouring the gas around it in the area known as the accretion disk, which leads to superheated conditions. This happens relatively close to the black hole, but the wind stirs a larger molecular outflow and the heat gives rise to a shock wave that ultimately clears out dust and gas in a much larger area. The study estimates that the outflow from this particular black hole extends up to 1,000 light-years from the galaxy’s center.
In other words, while busily feeding, a black hole is also “pushing away the dinner plate,” the report says. This finding provides astronomers with another piece of the puzzle regarding how black holes are connected to star formation in the galaxies that swirl around them.
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