“It appears that a supermassive black hole is explosively heating and blasting around the gas in this galaxy and, as a result, is transforming it from an actively star-forming galaxy into one devoid of gas that can no longer form stars,” said Chris Harrison from the Center for Extragalactic Astronomy at Durham University in the United Kingdom.
Two major types of galaxies are spirals, rich in gas and actively forming stars, and ellipticals, gas-poor and with very little star formation. The massive ellipticals, astronomers think, started life as active star-forming galaxies. Powerful jets and winds of material, powered by supermassive black holes at the galaxies’ centers, are believed to remove or destroy the raw material needed for continued star formation.
“For many years, we’ve seen direct evidence of this happening in galaxies that are extremely bright when viewed through radio telescopes. These rare radio-bright galaxies harbor powerful jets, launched at the black hole, that plow into the surrounding gas,” Harrison said. “However, to understand how all galaxies in our universe formed, we needed to know if these same processes occur in less extreme galaxies that better represent the majority. This was the focus of our study.”
As part of an ongoing investigation, Harrison and his colleagues used the VLA to study a galaxy labeled J1430+1339, also known as the “Teacup” because of its appearance. About 1.1 billion light-years from Earth, the galaxy had been identified as having characteristics typical of galaxies with a central black hole actively consuming material. Follow-up observations with NASA’s Hubble Space Telescope also revealed evidence that the Teacup has the appearance of an elliptical-type galaxy but is surrounded by gas that suggests it is still in the process of transforming from a star-forming galaxy.
The VLA observations showed that the galaxy has “bubbles” extending from 30,000 to 40,000 light-years on each side of its core, along with smaller jet-like structures about 2,000 light-years in size. These jet-like structures are located at the position where visible-light observations indicate gas is being accelerated to speeds up to about 620 miles per second (1,000 km/s).
Alasdair Thomson, another Durham astronomer involved in the study, said, “These radio observations have revealed that the central black hole is whipping up a storm at the center of this galaxy by launching powerful jets that are accelerating the gas in the host galaxy and are colliding with the gas on larger scales. This is the same kind of powerful process we’d previously seen in rare, extremely radio-luminous galaxies. The incredible capabilities of the VLA have allowed us to discover that these processes can occur in the more common radio-faint galaxies as long as you look hard enough.”
“This storm in the Teacup means that the jet-driven process in which a black hole is removing or destroying star-forming material may be much more typical than we knew before and could be a crucial piece in the puzzle of understanding how the galaxies we see around us were formed,” Harrison said.
Harrison and his collaborators now have observed eight more such objects with the VLA and are analyzing their data to see if the others show similar characteristics.
