The question of what triggers the extremely rapid star formation within Hyper Luminous Infrared Galaxies (HyLIRGs), as yet unknown, is of much interest to guide our understanding of the formation and evolution of galaxies in the Universe. A new photo released by the shows a HyLIRG 10,000 times brighter than our Milky Way (in infrared light) – the distant galaxy PJ0116-24 – and was released in conjunction with a newly published paper in Nature Astronomy that sheds light on its formation.
The distant galaxy PJ0116-24, a Hyper Luminous Infrared Galaxy (HyLIRG). Cold gas is seen here in blue; warm gas is shown in red.
Previous studies suggested that such extremely bright galaxies must result from . These galaxy collisions are thought to create dense gas regions in which rapid star formation is triggered. But isolated galaxies could also become HyLIRGs via internal processes alone, if star-forming gas is rapidly funneled towards the galaxy’s center.
In the paper, “,” on which Cornell astronomer , Ph.D. ’19, is a co-author, observations from ESO’s (VLT) and the (ALMA) were combined to study the motion of gas within PJ0116-24.
ALMA traces cold gas, seen in the photo in blue, whereas the VLT, with its new (ERIS), traces warm gas, shown in red. Thanks to these detailed observations, the international research team discovered that the gas in this extreme galaxy was rotating in an organized fashion, rather than in the chaotic way expected after a galactic collision — a surprising result. This shows, said the researchers, that mergers aren’t always needed for a galaxy to become a HyLIRG.
