A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-minute Period Variable Gaia22ayj
Date Issued
2025-02
Author(s) USM
DOI
10.1088/1538-3873/adb0f1
Abstract
White dwarfs (WDs) are the most abundant compact objects, and recent surveys have suggested that over a third of WDs in accreting binaries host a strong (B greater than or similar to 1 MG) magnetic field. However, the origin and evolution of WD magnetism
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