Speaker
Diego Altamirano
(University of Southampton)
Description
Black hole X-ray binaries (BHXBs) are key laboratories for studying accretion physics, relativistic jets, and strong gravity. Since its launch in 2017, NASA’s Neutron Star Interior Composition Explorer (NICER) has provided unprecedented X-ray timing and spectral data, enabling new insights into accretion phenomenology and the physics behind. In this talk, I will review what we have learned about BHXBs from NICER observations in recent years, highlighting key discoveries related to quasi-periodic oscillations (QPOS) and their link to relativistic jets. I will also summarize NICER major contributions to multi-wavelength campaigns.
Contribution | Oral talk |
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Affiliation | University of Southampton |
d.altamirano@soton.ac.uk |
Author
Diego Altamirano
(University of Southampton)