Constraints on Hadronic Emission from Microquasars Detected by LHAASO

arXiv:2606.29830 · astro-ph.HE · Submitted 2026-06-29 · Read on arXiv

V. Vecchiotti, E. Amato, G. Giacinti, G. Morlino, G. Peron

astro-ph.HE

Submitted: 2026-06-29

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Benchmark — 4× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Diffusion Model — 1× in this paper · explained in 8 episodes
• Large High-Altitude Air Shower Observatory — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Model of Cosmic Ray Propagation in the Milky Way at the Knee
• Unveiling Multimessenger Emission from Hidden Cores of Microquasars
• Microquasar Remnants as Pevatrons Illuminating the Galactic Cosmic Ray Knee

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2
• Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
• Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
• XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary