A possible evolutionary connection between high-mass X-ray binary pulsars and isolated rotation-powered pulsars

arXiv:2610.19595 · astro-ph.HE · Submitted 2026-10-14 · Read on arXiv

astro-ph.HE

Submitted: 2026-10-14

Updated: 2026-10-14

Comments: Accepted for publication in the Journal of High Energy Astrophysics

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

Related papers