Prefer a chat interface with context about you and your work?
<i>XMM</i>โ<i>Newton</i> campaign on ultraluminous X-ray source NGC 1313 X-1: wind versus state variability
Most ultraluminous X-ray sources (ULXs) are thought to be powered by neutron stars and black holes accreting beyond the Eddington limit. If the compact object is a black hole or a neutron star with a magnetic field $\lesssim10^{12}$ G, the accretion disc is expected to thicken and launch powerful winds โฆ