Exploring PSR J0901-4046 as an ultra-slowly rotating neutron star versus a white dwarf

astro-ph.HE

Submitted: 2026-10-20

Updated: 2026-10-20

Comments: 13 pages including 5 figures (14 png files) and 2 tables; accepted for publication in The Astrophysical Journal (ApJ) -- see Paper II as the companion paper titled: "Exploring the origin of slow-rotating pulsars: Emission from STARS simulated white dwarfs" also accepted for publication in The Astrophysical Journal (ApJ)

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

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
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• 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