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astro-ph.HE2025
Polarized Emission of Intrabinary Shocks in Spider Pulsars from Global 3D Kinetic Simulations
Andrew G. Sullivan, Jorge Cortés, Lorenzo Sironi
In spider pulsar systems, a relativistic intrabinary shock forms when the pulsar wind collides with the massive outflow driven off the pulsar's low-mass stellar companion. The shoc…
astro-ph.HE2025
Particle Acceleration and Nonthermal Emission at the Intrabinary Shock of Spider Pulsars. II: Fast-Cooling Simulations
Jorge Cortés, Lorenzo Sironi
Spider pulsars are binary systems composed of a millisecond pulsar and a low-mass companion. Their X-ray emission, varying with orbital phase, originates from synchrotron radiation…
astro-ph.HE2024
Particle Acceleration and Nonthermal Emission at the Intrabinary Shock of Spider Pulsars. I: Non-Radiative Simulations
Jorge Cortés, Lorenzo Sironi
Spider pulsars are compact binary systems composed of a millisecond pulsar and a low-mass companion. Their X-ray emission - modulated on the orbital period - is interpreted as sync…