Discovery of a 62-min long-period transient with near-orthogonal rotator geometry
astro-ph.HE
Submitted: 2026-09-28
Updated: 2026-09-29
Comments: 23 pages, 11 figures. Accepted for publication in The Astrophysical Journal
Code: https://github.com/AlecThomson/FixMS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- 3D-$N_{\rm H}$-tool
- The properties and origin of magnetic fields in white dwarfs
- Rotating Radio Transients
- Discovery of a 36-minute long-period transient ASKAP J142431.2-612611
- White dwarf + M dwarf Detached Binaries in Long Period Radio Transients: Observed Binary Parameters, Evolution, and Population Constraints
- Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary
- The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky
- FAST Pulsar Database IV. Spike subpulses and quasi-periodic subpulses of 25 pulsars observed by FAST
- VASTER: The ASKAP real-time fast-imaging pipeline -- overview and discovery of two long period transients
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
- 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