An article under review for publication reports a study on the galaxy ESO 253-G003 that classifies it among the ones with an active galactic nucleus that is consuming a star orbiting the central supermassive black hole. A team of researchers led by Anna Payne of the University of Hawaii used observations conducted with various telescopes to study the phenomenon, cataloged as ASASSN-14ko, detecting a series of regular cosmic outbursts that were interpreted as energy emissions linked to the passage of a star too close to the black hole, which destroys a part of it at each orbit.

An article published in “The Astrophysical Journal” reports a study on the galaxy CQ 4479, where a quasar was observed, an active galactic nucleus with a supermassive black hole that is devouring large amounts of matter, and at the same time an intense star formation. A team of researchers used the SOFIA flying telescope to observe CQ 4479, and found this situation called a cold quasar because the active galactic nucleus is very hot but the galaxy also contains cold gas that gives birth to new stars. This is a rare case that could show an astronomically short period in the evolution of a galaxy before the quasar starts inhibiting star formation.

An article published in the journal “Astronomy & Astrophysics” reports a study on hyperluminous galaxies. A team of researchers led by Lingyu Wang of the Netherlands Institute for Space Research, Utrecht, used the LOFAR radio telescope to assess the amount of hyperluminous galaxies in infrared and concluded that it’s ten times higher than what stars can produce according to current models. If the models are correct, it means that in many galaxies there are other light sources such as an active galactic nucleus powered by a supermassive black hole surrounded by large amounts of materials heated to the point of generating electromagnetic emissions.