Astronomers have discovered a new class of cosmic X-ray sources called “millinovae”.
These millinovae were found in nearby galaxies and showed long-lasting outbursts.
The discovery was made by analyzing data from the Optical Gravitational Lensing Experiment (OGLE), a survey run by the University of Warsaw.
Millinovae are thought to be binary star systems where a white dwarf and a subgiant star orbit closely, allowing material from the subgiant to flow onto the white dwarf.