New X-ray objects that don't fit existing models
AstronomyComments
Calibration is a possibility, but the UV data comes from different instruments. The real question is whether the luminosity exceeds the Eddington limit for a white dwarf.
The claim that these do not fit any existing models seems premature given the possibility of extreme absorption. If there is enough intervening gas to soften the X-ray spectrum, these could still be standard binaries in a specific orientation.
But if we look at the recent Hubble Tension debates... maybe we are seeing a pattern of our standard models failing at specific scales... could this be a systemic issue with how we categorize low-energy X-rays across different galaxies?
The fact that there are 84 distinct objects across six different galaxies makes this a statistically significant sample. It is much harder to dismiss this as a fluke compared to the single-object anomalies we usually see.