2 new star systems are first of their kind ever found

Prieto explained why. Over millions of years, a star will burn hotter or cooler as it consumes different chemical elements in its core. The most massive stars swing back and forth between being cool red supergiants or hot blue ones. They spend most of their lives at one end of the temperature scale or the other, but spend only a short time in-between, where they are classified as yellow. Most stars end their life in a supernova at the red end of the cycle; a few do at the blue end. But none do it during the short yellow transitional phase in between.

At least, that’s what astronomers thought.

Prieto, Stanek, and their colleagues suspect that yellow binary systems like the ones they found could be the progenitors of these odd supernovae.

“When two stars orbit each other very closely, they share material, and the evolution of one affects the other,” Prieto said. “It’s possible two supergiants in such a system would evolve more slowly, and spend more time in the yellow phase -- long enough that one of them could explode as a yellow supergiant.”

The discovery of this yellow supergiant binary system is just the first result of a long-term LBT project to monitor stellar variability in the nearby universe. That project is led by Ohio State professor of astronomy, Chris Kochanek. He and Rick Pogge, also a professor of astronomy, are coauthors on the paper in Astrophysical Journal Letters.

Their collaborators were from the University of Minnesota, the Osservatorio Astronomico di Padova, Steward Observatory, the Max-Planck-Institut für extraterrestrische Physik, the Osservatorio Astronomico di Roma, the University of Notre Dame, and the Large Binocular Telescope Observatory. They used observations from the 8.4-meter LBT and from the 2.4-meter telescope at the nearby MDM observatory.

The LBT is an international collaboration among institutions in the United States, Italy and Germany. The LBT Corporation partners are: the University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; Ohio State University; The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota, and University of Virginia.

This research was funded by the National Science Foundation.