Arp 299: Galactic Mash

Arp 299: Galactic Mash

What happens if you mix two galaxies for millions of years? A new snapshot from the Chandra Observatory will answer this question.

This is the Arp 299 system, which is 140 million light-years distant. It has two merging galaxies. In this process, new stars are created. However, the observations also show 25 x-ray sources. Moreover, 14 of them are powerful enough to become ultra-bright X-ray sources (SRI).

They are found in the regions of the active birth of stars. Most likely, we are dealing with binary systems, where a black hole or a neutron star steals matter from a neighbor that is more massive than the Sun. These are highly massive X-ray binary stars.

Such a cocktail is rare, but Arp 299 is one of the most powerful star-forming galaxies in the entire Universe. The reason was the merging of galaxies that activated stellar births. The composite image displays Chandra X-ray information (pink), NuSTAR high-energy X-ray data (purple), and visible observation of the Hubble telescope (white and weak brown). The system also emits a huge amount of infrared rays.

Interestingly, infrared and X-rays very much resemble examples of ancient galaxies. Chandra also displays diffuse X-rays from hot gas scattered throughout Arp 299. Most likely, the high speed of supernovae led to the fact that most of the hot gas left the system.

Comments (0)
Search