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Scientists Find Wind Blowing From Our Milky Way's Black Hole After Half-Century Search: 'There It Is'
A Northwestern University team used five years of ALMA data to map a cone-shaped cavity that suggests Sgr A* has been driving a wind for 20,000 years.
Northwestern University researchers announced they discovered a 20,000-year wind emanating from Sagittarius A* , the supermassive black hole at the center of the Milky Way, resolving a 50-year mystery.
Astronomers had searched for this release of material for 50 years, theorizing that active supermassive black holes expel gas; Sgr A*'s relatively quiescent phase made the outflow subtle and difficult to detect.
Using five years of observations from the Atacama Large Millimeter Submillimeter Array and NASA's Chandra X-ray Observatory, the team identified a cone-shaped cavity about 45 degrees wide, sculpted by the black hole's wind.
This finding confirms that Sgr A* behaves like other supermassive black holes, dispelling the idea that our galaxy's central anchor was an outlier, according to study co-leader Elena Murchikova of Northwestern.
Supermassive black holes are not isolated from their environments, according to co-author Mark Gorski, providing researchers a rare window into black hole behavior during its quiet, gentle state.