Accretion, ejection, and dynamical properties of X-ray binaries: from classical to ultracompact systems
Accreting black holes and neutron stars in X-ray binaries (XRBs) provide an ideal laboratory for studying compact object physics as well as the physics of accretionthe most efficient mechanism of energy production known. This project (XB-LAB), building on prior initiatives (AYA2017-83216-P, PID2021- 124879NB-I00, and PID2020-120323GB-I00) led by
Teodoro Muñoz Darias
Montserrat Armas Padilla
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