The Spin-Period History of Intermediate Polars
arXiv:2001.07288 · doi:10.3847/1538-4357/ab863d
Abstract
We report the detailed history of spin-period changes in five intermediate polars (DQ Herculis, AO Piscium, FO Aquarii, V1223 Sagittarii, and BG Canis Minoris) during the 30-60 years since their original discovery. Most are slowly spinning up, although there are sometimes years-long episodes of spin-down. This is supportive of the idea that the underlying magnetic white dwarfs are near spin equilibrium. In addition to the ~40 stars sharing many properties and defined by their strong, pulsed X-ray emission, there are a few rotating much faster (P<80 s), whose membership in the class is still in doubt -- and who are overdue for closer study.
arXiv commentPDF, 13 pages, 1 table, 2 figures; submitted, ApJ; more info at http://cbastro.org/
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