Astronomers have discovered a new class of “cold quasars” that could change our perception of how galaxies mature.
The discovery was announced at the annual meeting of the American Astronomical Society in St. Louis.
Cold quasars are galaxies that have an abundance of cold gas that is still able to produce new stars, despite having a quasar — a bright core powered by supermassive black holes — at its center. Gas falling toward a quasar at the center of a galaxy forms an accretion disk that can produce a large amount of electromagnetic energy and luminosity hundreds of times greater than a typical galaxy.
Typically, the formation of a quasar signals the end of a galaxy’s ability to produce new stars. But in the new research, about 10% of galaxies hosting accreting supermassive black holes still had a supply of cold gas and made new stars even during the so-called “retirement” phase.
“The quasars we have identified via their X-ray emission show a surprising amount of cold dust, more than was expected based on previous identification of quasars by their ultraviolet emission,” said co-author Meg Urry, the Israel Munson Professor of Physics and Astronomy and director of the Yale Center for Astronomy and Astrophysics (YCAA).
“The bottom line is, when you look in X-rays or infrared light, you find dustier, more obscured active galactic nuclei (AGN) than you find in optical or ultraviolet surveys,” Urry said.
The principal investigator is former YCAA Prize Postdoctoral Fellow Allison Kirkpatrick, who is now an assistant professor at the University of Kansas. The first author is Brandon Coleman from the University of Kansas. Additional co-authors include graduate student Tonima Ananna of Yale.
The research is part of a collaboration called the Accretion History of AGN, headed by Urry, that assembles archival data and carries out a multiwavelength analysis on it.
The researchers said the new finding may represent a brief phase of every galaxy’s lifecycle — akin to a retirement party — that was unknown until now. “These galaxies are rare because they’re in a transition phase — we’ve caught them right before star formation in the galaxy is quenched and this transition period should be very short,” Kirkpatrick said.
Source: Yale University