CORDIS Project
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This project investigates the behavior of neutron stars, particularly transitional millisecond pulsars, under extreme conditions. It focuses on understanding plasma outflows, mass accretion processes, and the formation of accretion disks through multi-waveband observations.
The behaviour of matter under extreme conditions and the reason why accretion onto many astrophysical objects is accompanied by outflows of plasma like jets, are key questions of astrophysical research.
Neutron stars (NSs) are prime laboratories for this investigation.
They are the solid-surface bodies in which the most extreme conditions of gravity, density, pressure and magnetization are realized.
When they are part of a binary system, and matter is transferred from their companion star, seve…
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