Research news on Ultraluminous x-ray sources

Ultraluminous X-ray sources (ULXs) as a research area focus on extragalactic, non-nuclear X-ray emitters with luminosities exceeding the Eddington limit of typical stellar-mass black holes, often in the range 10³⁹–10⁴¹ erg s⁻¹. This field investigates their nature as candidates for super-Eddington accretion onto stellar-mass compact objects or accretion onto intermediate-mass black holes. Research emphasizes multiwavelength observations, spectral and timing analyses, accretion physics in extreme regimes, the role of beaming and outflows, and their connection to star formation, X-ray binaries, and black hole growth across different galactic environments.

A nearby black hole as a window into the early universe

An international team led by Stefanie Komossa from the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn has studied a galaxy that has been shining exceptionally brightly in the radio regime for more than eight years. ...