Two colliding galaxies have spent millions of years slowly mixing and mingling their respective stars, resulting in a gorgeous interstellar stew filled with bright X-ray sources.

NASA's Chandra X-ray space telescope captured this stunning new view of the interacting galaxies, collectively named Arp 299, by observing the X-ray radiation emitted by this rich mix of stars.

The telescope spotted an unusually high number of bright X-ray sources in Arp 299. Of the 25 X-ray sources seen in the galactic mix, 14 are categorized as ultraluminous X-ray sources (ULXs) for their exceptionally strong X-ray emissions, NASA officials said in a statement. [When Galaxies Collide: Photos of Great Galactic Crashes]

"These ULXs are found embedded in regions where stars are currently forming at a rapid rate," NASA added. "Most likely, the ULXs are binary systems where a neutron star or black hole is pulling matter away from a companion star," a type of star system known as an X-ray binary. 

This composite image of the galactic merger Arp 299 combines X-ray data from NASA's Chandra X-ray Observatory (pink), higher-energy X-ray data from the Nuclear Spectroscopic Telescope Array, or NuSTAR (purple), and optical data from the Hubble Space Telescope (white/brown).
This composite image of the galactic merger Arp 299 combines X-ray data from NASA's Chandra X-ray Observatory (pink), higher-energy X-ray data from the Nuclear Spectroscopic Telescope Array, or NuSTAR (purple), and optical data from the Hubble Space Telescope (white/brown).
Credit: X-ray: NASA/CXC/Univ of Crete/K. Anastasopoulou et al, NASA/NuSTAR/GSFC/A. Ptak et al; Optical: NASA/STScI

 

While galaxies aren't usually packed with so many X-ray binaries, scientists believe that a wave of new star formation in Arp 299 is responsible for this abnormally dense population of these bright X-ray sources. 

The galactic merger that created Arp 299 also triggered a baby boom of stars as clouds of interstellar gas and dust from the original two galaxies collided. "The formation of high-mass X-ray binaries is a natural consequence of such blossoming star birth as some of the young massive stars, which often form in pairs, evolve into these systems," NASA officials said. 

To create this stunning, multicolor view of Arp 299, NASA combined data from the Chandra X-ray telescope with even higher-energy X-ray observations by NASA's Nuclear Spectroscopic Telescope Array (NuSTAR) and visible-light observations by the Hubble Space Telescope. 

The image was released on June 26, and astronomers detailed their observations in the Aug. 21, 2016, issue of the Monthly Notices of the Royal Astronomical Society.

Email Hanneke Weitering at hweitering@space.com or follow her @hannekescience. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.