Quasars are galaxies hosting supermassive black holes that radiate so much energy as they consume galactic debris that they heat up or expel gas that otherwise would be available for star formation, bringing the host galaxy’s growth to an end. But astronomers have now found a missing link of sorts, a so-called “cold quasar” in which star formation has managed to continue even in the presence of a ravenous supermassive black hole.
“This shows us that the growth of active black holes doesn’t stop star birth instantaneously, which goes against all the current scientific predictions,” said Allison Kirkpatrick, assistant professor at the University of Kansas in Lawrence Kansas and co-author of a study in The Astrophysical Journal. “It’s causing us to re-think our theories on how galaxies evolve.”
Kirkpatrick and her colleagues used the NASA-German Aerospace Center Stratospheric Observatory for Infrared Astronomy, or SOFIA, to study a quasar some 5.25 billion light years away known as CQ4479.
Infrared light emitted by dust that was heated up by the process of star formation, not the central black hole, allowed the researchers to estimate the rate of star birth over the past 100 million years, concluding CQ4479 is building about 100 Sun-size stars each year.
“SOFIA lets us see into this brief window of time where the two processes can co-exist,” said lead author Kevin Cooke, a postdoctoral researcher at the University of Kansas. “It’s the only telescope capable of studying star birth in this galaxy without being overwhelmed by the intensely luminous quasar.”
