Quasars are extremely bright and powerful sources of energy that sit in the centre of a galaxy, surrounding a black hole.
In systems with multiple quasars, the bodies are held together by gravity and are believed to be the product of galaxies colliding. It is very difficult to observe triplet quasar systems, because of observational limits that prevent researchers from differentiating multiple nearby bodies from one another at astronomical distances.
Moreover, such phenomena are presumed to be very rare.
This enabled them to find the triplet quasar, called QQQ J1519+0627.
The light from the three quasars has travelled 9 billion light years to reach us, which means the light was emitted when the universe was only a third of its current age.
Advanced analysis confirmed that what the team found was indeed three distinct sources of quasar energy and that the phenomenon is extremely rare.
Furthermore, no evidence was seen of any ultra-luminous infrared galaxies (galaxies with very strong emission in infrared light), which is where quasars are commonly found. As a result, the team proposes that this triplet quasar system is part of some larger structure that is still undergoing formation.
"Honing our observational and modelling skills and finding this rare phenomenon will help us understand how cosmic structures assemble in our universe and the basic processes by which massive galaxies form," Fumagalli said.
The study was published in the journal Monthly Notices of the Royal Astronomical Society.
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