Two long period radio transients are detached white dwarf-M dwarf binaries with matching periods, massive cool crystallized white dwarfs, low inclinations, and an estimated population of 100-2000 such systems within 2 kpc.
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5 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 5representative citing papers
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
CASM-256 is a new 256-antenna radio array at Owens Valley that uses real-time digital beamforming to search for fast radio bursts and galactic transients over a huge sky area.
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.
citing papers explorer
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A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
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Study for curvature radiation and magnetic pair creation process on polar-cap region of magnetic white dwarf
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.
- A Falsifiable Timing Test for the Double-White-Dwarf Model of Long-Period Transients