Portraits of the young and old in X-ray: New millisecond pulsar detections and updated characterization of young neutron stars

arXiv:2609.00176 · astro-ph.HE, astro-ph.SR · Submitted 2026-08-31 · Read on arXiv

astro-ph.HE, astro-ph.SR

Submitted: 2026-08-31

Updated: 2026-09-14

Terminology

• Accuracy — 2× in this paper · explained in 1 episode
• Chandra X-ray Center — 2× in this paper
• Abundance — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Chandra Interactive Analysis of Observations — 1× in this paper
• High Energy Astrophysics Science Archive Research Center — 1× in this paper
• Society of PhotoOptical Instrumentation Engineers — 1× in this paper

Sources

• A Search for X-ray Counterparts of Radio Pulsars

Related papers

• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• 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
• SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
• Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion