Massive black holes spewing out radio-frequency-emitting particles at near-light speed can block formation of new stars in aging galaxies¹, a study has found. The research provides crucial new evidence that it is these jets of "radio-frequency feedback" streaming from mature galaxies' central black holes that prevent hot free gas from cooling and collapsing² into baby stars.

 

"When you look into the past history of the universe, you see these galaxies building stars," said Tobias Marriage, assistant professor of physics and astronomy at Johns Hopkins and co-lead author of the study. "At some point, they stop forming stars and the question is: Why? Basically, these active black holes give a reason for why stars stop forming in the universe."

 

The findings have been published in the journal Monthly Notices of the Royal Astronomical³ Society. They were made possible by adaptation of a well-known research technique for use in solving a new problem.

 

Johns Hopkins postdoctoral fellow Megan Gralla found that the Sunyaev-Zel'dovich effect signature -- typically used to study large galaxy⁴ clusters -- can also be used to learn a great deal about smaller formations. The SZ effect occurs when high-energy electrons in hot gas interact with faint light in the cosmic microwave background, light left over from earliest times when the universe was a thousand times hotter and a billion times denser⁵ than today.

 

"The SZ is usually used to study clusters of hundreds of galaxies but the galaxies we're looking for are much smaller and have just a companion or two," Gralla said.

 

"What we're doing is asking a different question than what has been previously⁶ asked," Gralla said. "We're using a technique that's been around for some time and that researchers have been very successful with, and we're using it to answer a totally different question in a totally different subfield of astronomy."

 

"I was stunned⁷ when I saw this paper, because I've never thought that detecting the SZ effect from active galactic nuclei⁸ was possible," said Eiichiro Komatsu, director of the Max Planck Institute for Astrophysics in Germany and an expert in the field who was not involved in the research. "I was wrong. … It makes those of us who work on the SZ effect from galaxy clusters feel old; research on the SZ effect has entered a new era."

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