Laura Olivera Nieto,
Laura Olivera-Nieto
(Anton Pannekoek Institute for Astronomy, University of Amsterdam)
09/10/2025, 09:00
Plenary General
X-ray binary systems exhibiting jets (microquasars) have emerged as promising candidates to explain the observed cosmic-ray flux in the PeV energy range. A handful of microquasars are now known to emit multi-TeV radiation, implying in-situ acceleration of >100 TeV particles. In my talk, I will go over the existing very-high-energy (VHE) gamma-ray observations of these systems, with a focus on...
Gwenael Giacinti
(Tsung-Dao Lee Institute, SJTU)
09/10/2025, 10:00
Plenary General
Haocheng Zhang, Dr
Haocheng Zhang
(University of Maryland Baltimore County)
09/10/2025, 11:00
Kohta Murase
09/10/2025, 11:20
Plenary General
The recent diffuse gamma-ray and neutrino data support the multimessenger connection expected in hadronic scenarios. Microquasars have been of interest as very-high-energy gamma-ray emitters. We discuss implications of cosmic-ray ion acceleration in such objects as well as possible connections to active galactic nuclei.
Naomi Tsuji
(University of Tokyo/ICRR),
Paolo Coppi
09/10/2025, 11:40
